The galaxy presents as a slightly elongated, lenticular or early-type spiral with a prominent central bulge. The light distribution is centrally concentrated, indicating a higher density of older stars in the core region. A faint, diffuse disk is visible, with only subtle hints of spiral arm structure. The galaxy exhibits a relatively smooth appearance, suggesting a lack of significant recent star formation. Colors are consistent with a population dominated by older stars, with bluer hues concentrated in the outer disk and redder hues in the central bulge. There are no obvious signs of tidal interactions or mergers, although subtle distortions within the disk cannot be ruled out based on the available image resolution. Overall, this galaxy appears to be a moderately massive system, likely in a late stage of evolution.
