The galaxy exhibits a primarily smooth morphology with a noticeable degree of disturbance. The overall shape appears somewhat rounded. Evidence suggests an ongoing or recent merger event, with the core exhibiting some degree of disruption. The color profile indicates a yellow/red hue in the central region, shifting to more blue in the outskirts. This could indicate an older stellar population in the core, with younger, bluer stars forming in the outer regions perhaps as a result of interactions during the merger. No clear spiral arm structure is visible. The galaxy appears relatively compact.
