The galaxy presents as a relatively smooth, elliptical structure. It exhibits a high degree of central concentration with a bright, yellowish core, suggesting an older stellar population dominating the nucleus. The galaxy appears largely spheroidal, displaying a lack of prominent spiral arms or distinct features typically associated with disk galaxies. A faint, diffuse halo extends outwards from the central region. This halo has a slightly redder hue than the core. There is no evidence of strong tidal interactions or ongoing mergers. The overall morphology is consistent with an early-type galaxy.
