The galaxy presents a complex morphology indicative of an ongoing or recent interaction/merger event. A prominent, relatively linear feature extends from the main body of the galaxy, possibly representing a tidal tail or a disrupted spiral arm. This feature appears bluer in color, suggesting a population of younger, hotter stars relative to the core.

The main body of the galaxy exhibits a more amorphous structure, with clumpy regions of star formation visible. There is a suggestion of a disk-like component, viewed close to edge-on, but this is heavily distorted. The overall color of the main body is slightly redder compared to the extended feature.

The galaxy displays noticeable disturbances, indicating gravitational interactions are actively reshaping its structure. There are irregular clumps and asymmetries present, suggesting the influence of tidal forces and/or the accretion of smaller galaxies. The light from the galaxy indicates low star formation activity.
