The galaxy appears as a centrally concentrated object, with a largely smooth light distribution. The morphology is generally elliptical, with an approximate radius of 4.4 kpc. While primarily smooth, there is a slight indication of faint, disturbed features suggestive of a possible ongoing or past minor interaction. The primary body of the galaxy is largely spherical, with deviations in the outer edges that extend slightly away from the central spheroid. The core is noticeably brighter than its outskirts. The overall color is consistent with an older stellar population. Star formation appears subdued within the galaxy.
