The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical or potentially a lenticular type, displaying minimal discernible spiral arm structure. The central region exhibits a brighter, yellowish hue, suggestive of an older stellar population or dust obscuration. The outer regions transition to a bluer color, perhaps indicating the presence of some younger stars, though star formation activity seems generally low. The overall shape tends towards being rounded, with no significant tidal features or signs of major mergers evident. Minor disturbances cannot be ruled out but do not appear significant. The object subtends a small angular size, indicative of a significant distance. The lack of clear features implies a relatively quiescent evolutionary state.
