The galaxy presents a disk-like morphology, although with some apparent disturbances. It has a mostly smooth appearance with a fraction of clumpy features. The primary body is elongated, exhibiting a shape somewhere between round and cigar-shaped. There is evidence of tidal features suggesting a recent or ongoing interaction or merger event. The color distribution within the galaxy appears heterogeneous, with varying concentrations of light across the structure indicating differences in stellar populations and dust content.
