The galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction/merger event. The central region appears somewhat smooth, but with noticeable disturbances in its overall structure. A prominent feature is the presence of multiple distinct, bright components. These components appear to be connected by faint streams or bridges of material, indicating gravitational interaction between them. There is possible tidal debris or disrupted arms extending outwards from the main body of the galaxy. The galaxy exhibits a yellowish hue, possibly indicating a population of older stars and relatively low star formation activity. Overall, the galaxy displays evidence of a dynamic environment, likely influenced by gravitational interactions.
