The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits a slightly elongated, elliptical shape, appearing more "in-between" rather than perfectly round or cigar-shaped. The light distribution suggests a bulge-dominated system, with the brightest region concentrated at the core. There is faint evidence of a disk. The color is consistent with an older stellar population throughout the galaxy, with a relatively small amount of on-going star formation. The galaxy shows no obvious signs of significant tidal disturbances or major mergers.
