The galaxy presents as a concentrated, elliptical-like structure with a smooth, centrally-dominant light profile. The core appears intensely luminous, possibly indicating a high concentration of older stars or an active galactic nucleus, however there does not appear to be any extended or bright blue emission that would point to ongoing star formation in this region. The lack of spiral arm structures or dust lanes supports its classification as an elliptical galaxy. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. The even color distribution further points to a relatively quiescent evolutionary state.
