The galaxy exhibits a complex morphology, characterized by significant disturbances indicative of an ongoing or recent merger event. It presents a non-smooth appearance with clear features suggestive of tidal interactions. Evident are irregular extensions and disrupted structures. The overall shape is highly irregular, diverging from typical elliptical or spiral forms. The galaxy appears to be comprised of multiple interacting components, displaying an asymmetric distribution of light. Distinct regions show variations in color, with bluer hues concentrated in some areas, potentially indicating regions of recent or ongoing star formation. The overall low specific star formation rate suggests an older stellar population dominates, although the bluer regions may represent pockets of rejuvenated star formation activity.
