The galaxy presents a largely smooth and elliptical morphology. Its light profile suggests a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. The color appears generally redder, indicative of an older stellar population and lower levels of ongoing star formation. There is minimal evidence of spiral arm structure or significant dust lanes. The overall shape appears somewhat elongated, deviating slightly from a perfect circular form. Any potential tidal features or signs of recent mergers seem to be absent within the immediate vicinity of the galaxy.
