The galaxy exhibits a disturbed morphology, indicating potential interactions or mergers. The primary structure appears elongated, with an apparent central bulge and a diffuse halo. Distinct tidal tails or streams of stellar material extend outwards from the main body, suggesting ongoing or recent gravitational disruption. There are noticeable color gradients within the galaxy, with the central region exhibiting a slightly bluer hue compared to the outer regions. Star formation appears to be occurring, given the presence of relatively blue patches. Some regions appear more dusty, characterized by a slight reddening effect. The overall structure lacks a defined spiral arm pattern or a smooth elliptical shape. The system likely has a complex merger history.
