This galaxy presents an elongated morphology. The light profile shows a relatively smooth central region with a gradual decrease in surface brightness outwards. There are indications of some structural features or asymmetries in the outer regions, which may suggest minor disturbances or tidal interactions, although the overall structure appears relatively undisturbed. Color gradients are observed, with the central region exhibiting a yellowish hue, possibly indicative of an older stellar population, while bluer regions are discernible in the outskirts, potentially signaling ongoing star formation. The galaxy appears moderately bright, but with no highly distinct features. There is a suggestion of a weak disk-like structure with faint spiral arms that contribute to the overall irregular appearance.
