The galaxy presents as a relatively compact, lenticular-shaped object. Its light distribution appears centrally concentrated, with a smooth, diffuse halo surrounding a brighter core region. There is a suggestion of a disk-like structure, although it is not sharply defined. The elongation of the galaxy is evident, appearing more cigar shaped than perfectly round. There is a subtle colour gradient, with the central region appearing slightly bluer compared to the outer halo, which has a more reddish tint. This could be due to differential stellar populations, dust, or variations in star formation activity. There appear to be some minor disturbances. Further analysis, including higher resolution imaging and spectroscopic data, is required to ascertain the precise morphology, stellar populations, and any potential interactions or internal dynamic processes within the galaxy.
