The galaxy presents as a generally smooth object, with a slightly elongated, cigar-shaped morphology. A bright, somewhat centrally concentrated bulge region is observed. The color profile is suggestive of an older stellar population, with the central bulge appearing more blue. Fainter, diffuse outer regions extend from the central bulge. There is no significant evidence of strong spiral arm structure or a prominent disk, instead, its overall smoothness is evident. There is a hint of a minor disturbance.
