This galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk structure. The central region is characterized by a bright, concentrated core, suggesting a high stellar density or potential active galactic nucleus. Moving outward from the core, the luminosity gradually decreases, indicating a diminishing stellar population density.

The galaxy displays a color gradient, with the core exhibiting a yellowish-orange hue, which may be due to an older stellar population dominated by red giants and dwarfs. The outer regions exhibit a slightly bluer tint, possibly indicative of ongoing or recent star formation activity within a younger stellar population.

There is evidence of minor disturbances or irregularities in the outer regions, potentially suggesting a past or ongoing interaction with another galaxy. This is evident in the slight asymmetry of the galaxy's overall shape and the presence of faint tidal features extending from the main body. However, the overall structure remains largely undisturbed, indicating that any interaction has not resulted in a major merger event.

The galaxy appears to be relatively massive, based on its overall size and luminosity. The rate of star formation is low, which is expected for a galaxy of this morphology and age.
