The galaxy presents as a smooth, relatively featureless object with an elongated, cigar-like shape. Its color is predominantly a muted bluish-white, suggestive of a population of younger, hotter stars. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer edges of the galaxy. There is no evidence of spiral arms or a distinct disk component, and no significant dust lanes are apparent. The overall morphology suggests a galaxy that is likely undergoing minimal current star formation. Based on its structure it could be considered a lenticular galaxy type. There may be some indication of a minor gravitational disturbance of the galaxy, but overall it appears relatively unperturbed.
