The galaxy presents as a relatively smooth, elliptical structure. It is elongated, exhibiting an approximate cigar shape with a noticeable central bulge. The light distribution suggests a concentration of older stars, as indicated by its reddish-yellow hue, particularly within the central region. There is no apparent evidence of spiral arms or significant dust lanes. The overall morphology suggests a galaxy that is likely well-evolved, nearing the end of its star-forming activity. There are no obvious signs of ongoing major mergers or tidal disturbances.
