This galaxy appears to be an elliptical type galaxy, exhibiting a generally smooth and concentrated luminosity profile. The core is a bright, yellowish-white color, suggestive of an older stellar population. The galaxy exhibits a slight elongation, appearing somewhat football-shaped rather than perfectly spherical. Faint, diffuse emission extends outwards from the core in a more greenish halo, potentially indicative of some ongoing or recent star formation in the outer regions, although this could also be light from older stars at lower densities. There are no distinct spiral arms or bar structures visible. No strong signs of tidal disturbances or mergers are observed.
