The galaxy appears as a central bulge or spheroid of moderate luminosity with a bluer hue. This main body is surrounded by a less distinct, fainter, and more diffuse disk or halo of stars and gas, which is slightly elongated. There are indications of some mild disturbances or asymmetries in the outer regions, possibly suggesting past or ongoing interactions. It seems to be somewhat intermediate in shape between an elliptical and spiral, with a slight preference toward being in between round and cigar shaped. There are only minor disturbances in the morphology, and there is no clear evidence of a major merger event. Overall, the galaxy presents a relatively smooth, unperturbed structure.
