The object appears as a lenticular or early-type spiral galaxy at a redshift of approximately 0.085. It presents a predominantly smooth, rounded morphology, with a high concentration of light towards the central bulge region. There is the suggestion of a faint disk component and a single, prominent tidal tail extending from the core. The galaxy exhibits a color gradient, appearing bluer in the disk than in the central region. We estimate the galaxy is actively forming stars, based on the blue color of the tail. Overall, the galaxy appears to be relatively isolated with little evidence of recent major merger events.
