The galaxy presents as a moderately luminous, disk-shaped system with an apparent red shift. The central bulge is bright and appears mostly smooth, with no distinct spiral arm structure immediately visible within the central region. The disk exhibits a degree of asymmetry; one side appearing more extended. The overall morphology appears to favor a largely spheroid structure, although there is the suggestion of a fainter, outer disk or extended halo. The color distribution indicates a population that is primarily older, as evidenced by the redder hues, but there are hints of regions with more ongoing star formation. There appears to be a minor gravitational disturbance affecting the galaxy.
