The galaxy presents as a relatively small, yet well-defined system with evidence of a disk structure. The galaxy exhibits a moderate degree of disturbance, suggestive of ongoing interaction or past merger events. There appears to be a complex internal structure, with potential for spiral arm morphology, although this is obscured by the disturbances. The light distribution indicates active star formation, with a bias towards bluer wavelengths, and a detectable population of older stars contributing to the redder light. The galaxy's overall morphology indicates a system that is not completely relaxed.
