The galaxy appears to be a relatively smooth elliptical or lenticular type. It exhibits a bright, concentrated central bulge that dominates the overall light profile. The light appears to fade gradually outwards from the center, without any strong spiral arm features or obvious dust lanes visible in this image. The galaxy is somewhat elongated in shape, presenting an axial ratio less than 1. The galaxy is on the smaller side and appears relatively low mass. The object's color suggests that it might have a low star formation rate. There does not appear to be any signs of galactic mergers or tidal disturbances. 