The galaxy presents as a centrally concentrated object with a moderate degree of radial symmetry. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions show hints of spiral structure or disk-like features, though these are not sharply defined. There may be a slight dust lane along one edge, further obscuring the features. Irregularities are present within the galaxy's light distribution, potentially indicative of minor disturbances. The overall morphology appears somewhere between elliptical and early-type spiral, exhibiting properties of both. It has a relatively smooth light distribution. There appears to be ongoing star formation.
