This galaxy presents as a relatively compact, disk-shaped system with a noticeable central bulge. The galaxy exhibits a flattened morphology, viewed at an oblique angle, suggesting it is a spiral or lenticular type. The central region displays a bright, concentrated luminosity, indicative of a dense stellar population. A faint, diffuse halo extends outwards from the central region. There appears to be a ring-like structure with enhanced star formation. The light suggests ongoing star formation within the disk. There are no apparent signs of tidal disturbances or major mergers, although a slight asymmetry in the disk's outer regions cannot be ruled out as evidence of a minor interaction in the past. The overall color suggests the galaxy is composed of both younger, bluer stars and an older, redder stellar population.
