This galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated bulge that dominates its overall structure. The light distribution suggests it is an evolved system, and the object is observed at redshift z = 0.201921. The galaxy displays a weak disk structure with a slight elongation, suggesting a cigar-like shape. The lack of prominent spiral arms indicates a relatively low star formation rate overall, consistent with the color profile being dominated by older stellar populations with a significant red component. There is a possible minor disturbance on the edge of the disk, but there is no conclusive sign of any major ongoing merger activity.
