The galaxy presents as an elliptical morphology with a concentrated central bulge. The light distribution appears relatively smooth, without obvious spiral arm structures. The color gradient suggests a mature stellar population, with the central region exhibiting a yellowish hue potentially indicative of older stars. There are no prominent dust lanes or active star forming regions visible. The galaxy appears somewhat disturbed with hints of tidal features, perhaps resulting from a past or ongoing interaction with a smaller companion galaxy. The overall size of the galaxy appears substantial relative to other objects in the field.
