The galaxy presents as a relatively compact, flattened system. It exhibits a smooth light distribution, with a concentrated central region that gradually fades towards the edges, suggesting a dominant bulge component. The galaxy's shape appears to be somewhere between perfectly circular and elongated. There might be some minor disturbances in its morphology, but the galaxy does not appear to be undergoing a major merger or exhibiting strong tidal features. Overall, the galaxy presents a classic disk-like morphology with evidence of bulge dominance. It exhibits blue color, which implies the presence of young stars and recent star formation activity, though at a moderate rate, given its mass.
