The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge of yellowish-white light, suggesting an older stellar population. A slight extension of diffuse light surrounds the central bulge, possibly indicating an extended stellar halo. There is a very slight suggestion of a disk-like structure, but the overall morphology is dominated by a spheroidal shape. There's no visible evidence of spiral arms or active star formation regions. The galaxy is slightly elongated, but not significantly cigar-shaped. There is no indication of any major mergers or significant tidal disturbances.
