The galaxy presents as a relatively compact object with a concentrated central bulge. The light distribution appears predominantly smooth, suggesting a lack of significant spiral arm structure or prominent dust lanes. The galaxy exhibits a slightly elongated shape, appearing somewhat intermediate between perfectly round and cigar-shaped. A faint, diffuse halo seems to extend beyond the central region. There are no obvious signs of recent major merger activity, although a subtle asymmetry or minor disturbance on one side is not ruled out. The galaxy's color indices indicate a moderately red population, consistent with older stars and potentially lower rates of ongoing star formation. Overall, the galaxy appears to be a moderately massive early-type system at intermediate redshift.
