The galaxy presents as a somewhat elliptical object with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars and potentially a supermassive black hole actively accreting material. The outer regions appear fainter and exhibit a slightly bluer tint, hinting at the presence of younger, hotter stars and ongoing star formation, although at a relatively subdued rate.

There is a suggestion of minor disturbances in the galaxy's overall morphology, possibly indicative of a past or ongoing minor interaction or merger event. This is seen as a slight asymmetry in the light distribution.
