The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The overall shape is elliptical, displaying a high degree of circular symmetry. The core region exhibits a yellowish hue, suggestive of an older stellar population. Fainter, bluer light is present in the surrounding regions, possibly indicating some ongoing, albeit low-level, star formation. There is no discernible spiral arm structure or significant dust lane features visible. The galaxy does not appear to be undergoing any major merging activity or tidal disruption, appearing as a relaxed system.
