The galaxy appears to be a relatively bright, elliptical galaxy exhibiting a smooth, centrally concentrated morphology. Its color profile suggests a population dominated by older stars, indicated by a yellowish-red hue towards the core, which slowly fades into a redder outer halo. The galaxy presents a moderate level of roundness, showing a slight flattening. There are no readily apparent signs of spiral arm structures, prominent dust lanes, or major tidal disturbances, suggesting that this galaxy is likely not undergoing any recent major mergers or intense star-forming activity.
