The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable bulge. The overall morphology appears elliptical or lenticular, displaying a high degree of symmetry. The galaxy exhibits a yellowish-red hue, suggestive of an older stellar population and a diminished rate of recent star formation. There is a subtle color gradient, where the core is more yellow/red than the extended area. The galaxy does not appear to have any spiral arm structures, a bar, or significant dust lanes. No obvious tidal features or close companion galaxies are apparent in its immediate vicinity, despite the minor disturbances reported in its morphology data. The smooth appearance indicates a possible history of mergers or interactions, which may have contributed to its current form.
