The galaxy appears as a somewhat elongated, lenticular or early-type spiral structure at an estimated distance corresponding to a redshift of approximately 0.275. The overall color is noticeably blue, suggesting ongoing star formation. The galaxy exhibits a smooth, yet slightly disturbed morphology, possibly indicative of a minor interaction or past merger event. Faint hints of a disk-like structure can be discerned, but a prominent central bulge dominates the overall light distribution. There are no apparent strong tidal features or signs of a major ongoing merger. The galaxy is moderately luminous, potentially residing within a group or cluster environment given its apparent mass.
