The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its morphology is largely spheroidal, showing minimal evidence of a prominent disk or spiral arms. The object appears approximately round in shape. There are no signs of tidal tails or other significant disturbances suggestive of recent major merger activity.

The galaxy exhibits a color gradient, appearing yellower toward its core and slightly bluer in its outer regions. This color difference may imply varying stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars possibly present in the outer halo. The low overall star formation rate is generally consistent with an older stellar population. The galaxy is a single, well-defined object, exhibiting no clear signs of multiple nuclei or other features typically associated with ongoing mergers.
