The galaxy presents as an elliptical or lenticular structure, with a relatively smooth light distribution, where the light is concentrated towards the center and decreasing outwards. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint, perhaps indicating the presence of younger stars or ongoing star formation, though subdued. There is a slight asymmetry observed in the shape of the galaxy. It does not appear to be a pure elliptical, and possibly has an inclination, indicating there may be a small disk-like structure. There does not appear to be any spiral arm structures visible.
