The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge that dominates its overall luminosity. There is minimal evidence of spiral arm structure or prominent dust lanes. The galaxy appears to be somewhat spheroidal in shape, with a slight elongation. The color gradient suggests an older stellar population, with a yellowish-orange hue concentrated towards the core, indicating a likely lower rate of current star formation. There are faint indications of an extended halo, gradually fading into the background sky. There is no visible evidence of an ongoing merger or major tidal disturbances. The overall structure implies a galaxy which has largely completed its morphological evolution, and has a large mass.
