The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears spheroidal, gradually fading into a diffuse halo. The color profile is primarily red-shifted, suggestive of an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a quiescent, relatively evolved system. Possible minor disturbances may be present in the outskirts, but no large-scale mergers are readily apparent. The light distribution suggests a fairly regular shape, deviating only slightly from a perfect ellipse.
