The galaxy appears as an elongated, cigar-shaped structure with a clear axis of elongation. The light distribution is not uniform; a brighter, more concentrated central region is noticeable, potentially indicating a galactic bulge. The overall color is yellowish-white, which implies a population of older stars and a moderate amount of ongoing star formation. There is a slight indication of a disk component, but it is not clearly defined. A minor disturbance may be present on the right side of the galaxy. It is difficult to determine if the galaxy is isolated or if there is a companion galaxy interacting with it. 