The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a defined disk structure. The central region exhibits a brighter, more concentrated luminosity, suggesting a possible galactic nucleus or bulge. A gradual decrease in light intensity is observed moving outwards from the center, with no sharp edges or boundaries visible.

The color profile displays a central orange-red hue, indicative of an older stellar population. The outer regions exhibit a slightly bluer tint, suggesting the presence of some younger stars, but overall the dominant color points towards a population of older stars.

There might be a hint of minor disturbance present. There is a possible close companion, which could be a source of interaction. Overall, however, this is likely an evolved galaxy.
