The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge, with a gradual decrease in luminosity extending outwards. There is no apparent spiral arm structure or distinct features indicative of ongoing major mergers. The color appears yellowish-orange, suggesting a stellar population dominated by older, redder stars and relatively low levels of recent star formation. The roundness of the galaxy indicates it may be close to an E0 classification based on ellipticity. Minimal signs of dust lanes or patchy star formation regions are observed.