The galaxy exhibits a centrally concentrated, elliptical morphology. The core region is bright, with a gradual decline in luminosity moving outwards. The galaxy appears to be largely spheroidal, with minimal visible disk-like features. There is a smooth, diffuse halo surrounding the main body of the galaxy. Color gradients are subtle but present. The central bulge exhibits a yellower hue, while the outer regions may be slightly bluer. No strong evidence of spiral arms, active star formation regions, or significant dust lanes are apparent. The overall appearance suggests an evolved galaxy, likely dominated by an older stellar population. There are no clear indications of recent merger events, but some minor asymmetry cannot be ruled out.
