The galaxy presents as a relatively compact, elliptical-like structure with a smooth light profile, indicating a lack of significant spiral arms or prominent disk features. It is characterized by a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars.

A subtle bluer region is visible on the bottom part of the galaxy. This may be a sign of ongoing star formation activity, although it is not a very large portion of the galaxy. There are small indications of a possible minor interaction or disturbance, given the slight asymmetry in its morphology. There also appears to be another object next to it, which may or may not be related to this galaxy. Based on the light profile and color, it could be a companion galaxy.
