The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a notable central bulge, which appears brighter and more yellow/gold in color, suggesting a higher concentration of older stars. The isophotes are elongated, and the galaxy appears to be more of an in-between shape as opposed to perfectly round. There's little evidence of spiral arms or significant dust lanes. The outer regions of the galaxy appear fainter and slightly bluer, implying some younger stellar populations, though the overall color profile suggests an evolved stellar population. There is no obvious major tidal disturbance or signs of a major ongoing merger.
