The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. Extending outwards from the core is a fainter, more diffuse halo or disk. The lack of distinct spiral arms or significant dust lanes indicates that star formation rates are likely subdued within the galaxy. There are no signs of major morphological disturbances or tidal features, indicating no recent major mergers, although minor interactions cannot be ruled out. The overall shape appears to be somewhat flattened, leaning away from a perfect sphere. The galaxy's color profile indicates a larger population of older stars, suggesting it is an early-type galaxy, likely an elliptical galaxy with a large mass. 
