The galaxy presents as a generally smooth object, likely an elliptical or lenticular galaxy given the lack of discernible spiral arm structure. Its shape is somewhat rounded, though not perfectly spherical, exhibiting a moderate degree of ellipticity. There is no strong visual evidence of major mergers or significant tidal disturbances impacting its overall morphology, though minor asymmetries may be present. The color profile suggests a population of older stars, with a yellow-red hue dominating the central region, shifting towards a faint greenish tinge as it extends outward. This coloration is indicative of a lower star formation rate and a stellar population that has aged significantly. The galaxy is relatively compact, spanning a moderate angular size on the sky.
