The galaxy exhibits a complex morphology suggestive of a disturbed system. The light distribution is not uniformly smooth; rather, the central region presents a mixed profile. The overall shape appears elongated, possibly indicative of a disk-like structure viewed at an angle. There appears to be internal structure, with hints of spiral arms, although they appear disorganized and fragmented.

The galaxy displays variations in color. The central region is primarily red, while the outer regions show a more blue tint. The red hue in the core may be due to a population of older stars or significant dust obscuration. The bluer outer regions may indicate regions of active star formation.

There is evidence of tidal features or distortions. These faint and wispy structures could be indicative of past or ongoing gravitational interactions with another galaxy. It could also be a sign of a recent merger event.
