The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The light distribution suggests a somewhat elongated shape, approaching a cigar-like morphology. A color gradient is observable, transitioning from a yellowish-white core to a bluish outer halo, potentially indicative of differing stellar populations or dust distribution. There are no apparent signs of significant tidal interactions or major mergers in its immediate vicinity. The galaxy exhibits a smooth, featureless disk, possibly composed primarily of older stars.
