The galaxy appears to be an early-type spiral or lenticular galaxy observed at redshift z ≈ 0.2, corresponding to a lookback time of approximately 2.5 billion years. It is centrally concentrated, exhibiting a prominent bulge component that is elliptical in shape and yellowish in color. The bulge dominates the overall light profile. The spiral arms or disk are faint and not well-defined, showing a bluer hue than the bulge. There are no obvious signs of major mergers or strong tidal disturbances. The light distribution is relatively smooth, and there is no pronounced evidence of ongoing star formation in the central regions. Based on the colors, some star formation may be occuring in the disk region.
