The galaxy presents a generally smooth morphology, with a dominant central bulge. The overall shape appears elliptical, elongated along one axis, with a minor cigar shape. The light distribution is centrally concentrated. The color gradient suggests that the central region is composed of older stellar populations. There is very weak evidence of a spiral arm structure. Possible minor disturbances or interactions cannot be ruled out, but there are no clear signs of major mergers or tidal features. There is a lack of significant star formation regions or dust lanes.
