This galaxy exhibits a complex morphology indicative of ongoing or recent gravitational interactions. The primary body appears to be a spiral galaxy seen at an oblique angle, displaying a discernable but not well-defined disk structure. There is a clear tidal arm or bridge extending from the disk, suggesting a gravitational disturbance.

Color gradients are present, with bluer hues concentrated in the arms/disk region and a more yellowish/reddish hue in the central bulge, potentially indicating differing stellar populations. There is a secondary, more compact object in close proximity to the primary galaxy, possibly a dwarf galaxy, that appears to be interacting with the primary spiral.

Additionally, there is a noticeable distortion in the overall shape, possibly a result of ongoing merging or tidal interactions with the nearby compact object. Overall, this galaxy displays characteristics consistent with a merging system or a galaxy undergoing tidal disruption.
