The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears slightly elongated. The color profile suggests a population of older stars, with a yellowish to reddish hue dominating the galaxy's overall appearance. There is little evidence of significant dust lanes or prominent spiral arms. The light is distributed in a somewhat even fashion, with a gradual decrease in intensity from the core outwards. There is some evidence of low-level ongoing star formation. The galaxy appears fairly isolated, showing no immediate signs of major interaction or merging with other significant galaxies, although there could be minor disturbances occurring. It displays a generally relaxed morphology, consistent with a galaxy that has undergone significant dynamical evolution.
