The galaxy presents a predominantly smooth morphology, indicative of an elliptical galaxy. It exhibits a slightly elongated, cigar-shaped structure, but its deviation from circularity appears subtle. The core region is notably bright, with a yellow hue suggestive of an older stellar population. The galaxy displays a radial decrease in surface brightness from the center. There are no visible spiral arms, dust lanes, or indications of active star formation regions within the galaxy itself. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, though the possibility of minor interactions cannot be excluded based on this image alone. Its overall smooth and relatively featureless nature suggests it is a relatively evolved system.
