The galaxy appears to be an interacting system, potentially in the early stages of a merger. Two distinct luminous components are visible. One component exhibits a more elongated, cigar-shaped morphology, possibly a disk galaxy seen at an oblique angle. The second component appears more rounded and diffuse. The overall color of the galaxy appears to be reddish-yellow, suggesting a population of older stars and a relatively low rate of on-going star formation. There is a suggestion of tidal distortion or a bridge of material connecting the two components, but the image resolution makes it difficult to definitively confirm. There is no obvious presence of strong spiral arm structure or dust lanes in either component.
