The galaxy exhibits a disturbed morphology, suggesting a potential interaction or merger event. It appears elongated, with a noticeable "cigar" shape. The light distribution suggests a centrally concentrated bulge, with a relatively smooth profile but it could also be two separate galaxies. There is evidence of faint features extending from the main body. The overall color is moderately red, indicating a population of older stars and potentially lower current star formation rate. The galaxy is relatively compact.
