The galaxy presents as a centrally concentrated, elliptical-like morphology with a smooth appearance. It exhibits a relatively high degree of rotational symmetry, appearing nearly circular from our viewing angle. There is some indication of a possible minor disturbance of the main body as the galaxy appears to be interacting with a smaller system. The primary body of the galaxy exhibits a yellowish color, suggestive of an older stellar population, with little evidence of ongoing significant star formation. There appears to be a long tail of distortion as well, possibly indicative of more of a merger.
