The galaxy presents as an elliptical morphology, appearing largely featureless and smooth. The core exhibits a concentrated brightness, indicative of a substantial stellar population, likely older stars. The isophotes are generally elliptical, with the major axis appearing only slightly elongated. The color profile suggests a redder central region, possibly due to a higher concentration of older, cooler stars or dust obscuration. The outer regions show a gradual decrease in luminosity, fading into the background sky. There is no apparent spiral arm structure or distinct dust lanes. The galaxy exhibits minimal signs of ongoing mergers or tidal disturbances, presenting as a relatively isolated and relaxed system.
