The galaxy presents as a predominantly smooth, elliptical-like structure with a concentrated central bulge. The light profile appears centrally peaked and diminishes gradually toward the outer regions of the galaxy. The galaxy exhibits a yellow/red hue, suggestive of an older stellar population. There is no clear evidence of spiral arm structure or significant dust lanes. Faint hints of blue may be present in the outer edges, which could be from small populations of hot, young stars. The overall impression is of a relatively evolved system with little active star formation occurring presently. There are only minor signs of any current or past galactic mergers or tidal disruptions to the galaxy.
