The galaxy presents an elliptical morphology, appearing as a smooth, somewhat elongated structure. The central region exhibits a bright, concentrated luminosity, indicative of a high stellar density, potentially a galactic bulge. Moving outwards from the core, the light intensity decreases gradually, suggesting a smooth transition into the outer regions of the galaxy. There is a subtle color gradient detectable within the galaxy. The core appears to have a slightly yellower hue, possibly indicating a population of older stars. The outer regions show a hint of bluer light, which might reflect the presence of some younger, hotter stars, although this is less prominent. There is no clear evidence of distinct spiral arms or significant dust lanes. The overall appearance suggests a relatively evolved system.
