This galaxy presents as a centrally concentrated object with a smooth overall appearance. The central region exhibits a diffuse, reddish glow, possibly indicative of an older stellar population or significant dust obscuration. Extending outward from the core is a bluer, more diffuse halo or disk-like structure. This suggests the presence of younger stars, potentially within a disk component undergoing star formation. The galaxy's shape appears somewhat elongated, with an axis ratio that indicates it is not perfectly circular, though neither is it highly elongated. There is no clear evidence of spiral arms or strong tidal features, and the overall morphology suggests a lack of significant recent merger activity. A slight asymmetry is potentially visible in the distribution of the outer disk/halo, which may be indicative of a minor interaction or internal disturbance, but it is not pronounced.
