The galaxy presents a generally smooth and elliptical morphology. There is little to no evidence of spiral arm structure, with the light distribution appearing diffuse and centrally concentrated. Its color is relatively red, suggestive of an older stellar population and/or dust obscuration. The object appears relatively isolated, without strong signs of ongoing or recent major merger events. It exhibits a cigar shape. There might be signs of a minor disturbance within the disk, but it is hard to tell for sure.