The galaxy presents as a centrally concentrated, relatively smooth, and round structure. It exhibits a distinct yellowish hue, suggesting a dominant population of older stars. There is little evidence of spiral arms or prominent dust lanes. The galaxy appears to be moderately elliptical in shape. There are no indications of any major mergers or significant tidal disturbances, although a slight asymmetry cannot be entirely ruled out. The overall morphology points towards an early-type galaxy, potentially an elliptical or lenticular type.
