The galaxy presents as a primarily smooth object, lacking distinct spiral arm structures or prominent dust lanes. Its morphology appears to be elliptical, exhibiting a cigar shape rather than a perfect circular form. There is a slight elongation visible. The galaxy's color index suggests a population of older stars, contributing to its somewhat redder appearance. There are no obvious signs of major mergers or significant tidal disturbances in this image. The galaxy appears to be relatively isolated, without close companion galaxies or evidence of ongoing interactions.
