The galaxy presents as a diffuse, centrally concentrated object with a generally smooth appearance. There is no apparent spiral arm structure or distinct dust lanes visible. The light is a somewhat uniform hue of pale blue. There appears to be an extended halo of light surrounding the central bulge. The object does not appear perfectly circular, showing a slight elongation or distortion. Close inspection reveals some subtle irregularities in the outer regions, possibly indicating minor gravitational interactions or ongoing accretion events.
