The galaxy presents as a relatively smooth, centrally concentrated object. It is observed to be elliptical in shape, appearing mostly round, with only a slight deviation toward a cigar shape. The light profile suggests a bulge-dominated morphology.

The galaxy exhibits a yellowish-white hue, indicative of a relatively older stellar population, particularly in the central bulge. There is a subtle color gradient, with the core region appearing more yellow and the outer regions showing a slightly bluer tone. This may suggest some ongoing, though limited, star formation in the outer regions. No distinct spiral arms or features of active star formation regions are visible. Overall, the galaxy appears to be relatively quiescent with a low star formation rate. There is no significant evidence of tidal disturbances or ongoing mergers.
