The galaxy presents as a moderately luminous, disk-shaped structure, elongated along its major axis. The central bulge is prominent and exhibits a smooth, concentrated luminosity profile, suggesting a substantial population of older stars. The disk component appears less defined, with a smoother texture and a subtle color gradient from the inner regions outward. One side of the disk shows a slightly bluer tint, potentially indicative of ongoing or recent star formation. The overall shape is somewhat cigar-like, lacking any signs of strong spiral arm structure or significant morphological disturbances, possibly suggesting the later stages of its evolution. There appears to be no strong evidence of an ongoing merger or major tidal interaction in the immediate vicinity of the galaxy.
