The galaxy exhibits a predominantly elliptical morphology, appearing largely smooth and spheroidal in shape. It displays a concentrated central bulge that graduates to a less concentrated halo. Evidence of a faint, diffuse disk-like structure may be present. The galaxy's color profile suggests a predominantly older stellar population. A slight color gradient is observed, with the central bulge appearing more yellow-orange and the outer regions exhibiting a bluer hue. No signs of ongoing major mergers are apparent; however, subtle disturbances cannot be entirely ruled out, but nothing is particularly visible.
