The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core presents a yellowish-orange hue, potentially indicative of an older stellar population. A surrounding, less luminous halo graduates outward from the core, displaying a bluer color, which may suggest the presence of younger stars or ongoing star formation, although the rate of star formation seems relatively low. The galaxy's shape is moderately elliptical, leaning towards round. There is no obvious evidence of significant tidal disturbances or major mergers in the immediate vicinity, although a slight asymmetry in the outer halo could point to a minor interaction or past merger event. Overall, the galaxy seems to be a fairly massive, evolved system with a substantial stellar mass.
