The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. The main body of the galaxy appears elongated, with a cigar-shaped structure. There is an apparent tidal feature extending from one end, presenting as a bluer region compared to the main body of the galaxy. The bluer color suggests a population of younger, hotter stars in this region.

The central region exhibits a yellower hue, potentially indicating an older stellar population or the presence of dust. There's also a faint, diffuse halo extending around the galaxy. Overall, the galaxy appears to be in a dynamic state.
