The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a bright core, suggestive of a high stellar density. The overall color profile indicates a population of older stars, with a tendency towards redder hues in the central region, fading into slightly bluer tones at the outer edges. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy does not display any obvious signs of ongoing major mergers or tidal disturbances, it exhibits a well-defined, round morphology, suggesting relative dynamical stability. 
