The galaxy presents as a lenticular or possibly a spiral galaxy viewed edge-on. It exhibits a relatively smooth, elongated morphology with a bright central bulge. The bulge appears somewhat rounded. The disk component, while not highly resolved, seems prominent with a slight blue hue suggestive of some ongoing, though possibly subdued, star formation. There are no obvious signs of major tidal disturbances or ongoing mergers with other galaxies, though a minor interaction cannot be entirely ruled out. The overall color profile indicates a population dominated by older stars, especially within the central bulge.
