The galaxy presents as a diffuse, centrally concentrated object with a relatively smooth morphology. Its overall shape is generally elliptical, appearing more "in-between" than perfectly round or cigar-shaped. The light distribution suggests a lack of significant spiral arm structures or prominent star-forming regions. There is no evidence of any major mergers or significant tidal disturbances within the observable structure of the galaxy, although some minor disturbances may be present. The light appears more red than blue, hinting that it is more massive, and is likely to be a later-type galaxy.