The galaxy appears to be a relatively large, disk-shaped system, seen nearly edge-on. A prominent central bulge is evident, exhibiting a yellowish-orange hue, which may indicate an older stellar population. The disk itself appears fainter and displays a bluer color, potentially suggesting ongoing star formation. The disk shows possible signs of disturbance. There appears to be some tidal distortions and asymmetries in its morphology, possibly due to interactions with other galaxies. These disturbances could suggest that the galaxy is undergoing, or has recently undergone, a minor or major merger event. The galaxy has an estimated high mass and moderate star formation rate. The overall structure can be classified as an actively merging system.
