The galaxy presents as an elongated, cigar-shaped structure. Its overall color is a warm yellow-orange, suggesting a population of older stars and potentially a lower rate of current star formation. The light distribution within the galaxy appears relatively smooth, with a gradual decrease in brightness from the central region outwards. There is a subtle irregularity observed on one end of the galaxy which may indicate the presence of tidal features or perhaps a minor disturbance. It appears that the galaxy is not undergoing any major merging activity.
