The galaxy appears as a roughly elliptical structure with a bright, concentrated central bulge. The overall color profile suggests ongoing star formation, particularly within the central region and extending outwards into a faint, diffuse disk. There is a suggestion of a tidal tail or disrupted structure to the left of the galaxy, indicating possible past interactions or ongoing accretion events. The disk itself is relatively smooth in appearance, showing little evidence of strong spiral arm structure. The galaxy's relatively small angular size implies that it is a distant object. There is a slight asymmetry in the halo.
