The galaxy appears to be a smooth, elliptical type. It exhibits a somewhat elongated, cigar-like shape. The central region displays a bright, yellowish-white hue, which suggests a population of older stars. The outer regions of the galaxy fade gradually into the background, showing a subtle reddish-orange tint. There is no apparent presence of spiral arms or significant dust lanes. Based on the observed morphology, this galaxy shows little evidence of recent or ongoing major mergers or disturbances.
