The galaxy presents as a somewhat flattened spheroid, displaying a smooth, elliptical morphology. Its overall color profile indicates a population of older stars, with a general lack of prominent blue star formation regions. The galaxy is not perfectly circular, exhibiting a moderate degree of ellipticity. There is no prominent disk or spiral arm structure visible. The luminosity profile appears concentrated towards the galactic center, with a gradual decrease in brightness towards the outer edges. Slight disturbances are observed on the edge of the object. There are hints of possible interactions or mergers, but without more data, I cannot confirm. The galaxy is not extremely bright, suggesting either a relatively low stellar mass or a substantial distance.
