The galaxy presents as a moderately luminous, elongated structure. It exhibits a relatively smooth morphology, suggesting a lack of significant recent or ongoing major mergers or tidal disturbances. The light distribution indicates a central bulge that is brighter than the surrounding disk. The disk component appears somewhat flattened, contributing to the elongated shape of the galaxy.

Color gradients are subtle. There is an indication of bluer colors in the outer disk region, potentially indicative of ongoing star formation. The overall color profile suggests a relatively evolved stellar population. There is a slight asymmetry in the light distribution, but no clear signs of strong tidal tails or distortions in the disk. The overall impression is of a relatively undisturbed system undergoing slow, steady star formation.
