The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. There is a slight indication of some disk-like structure, but it is poorly defined. The color profile suggests a population of older stars, dominated by redder wavelengths. No prominent spiral arms or active star forming regions are discernible. There is a minor visual disturbance. It seems more likely to be a minor disturbance rather than a full on merger.
