This galaxy presents as a relatively smooth, elongated structure. It exhibits a central bulge that appears brighter and more concentrated, with a diffuse halo extending outwards. The galaxy appears somewhat cigar-shaped, lacking a well-defined spiral arm structure. The color gradient suggests a possible concentration of older stars, but does not definitively show that it has ended star formation. Some minor asymmetry or disturbance may be present in the outer regions of the galaxy.
