The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated morphology. It is mostly spheroidal in shape, though it shows some flattening and elongation. The light distribution gradually decreases from the center outwards, with no readily apparent spiral arms or distinct features. The core region appears yellowish, suggesting a population of older, redder stars dominating this area. Further out, there is a gradual transition to a greenish hue, likely due to the presence of younger, bluer stars, possibly indicative of some star formation activity. The outer edges of the galaxy gradually fade into the background, exhibiting a diffuse halo. There is no strong evidence of any major mergers or tidal disturbances in the immediate vicinity. The galaxy seems relatively isolated.
