The galaxy appears to be a relatively compact object, exhibiting a moderate degree of ellipticity. The central region displays a high surface brightness, with a concentrated, yellowish-white core. Moving outwards from the core, the light appears to gradually fade into a more diffuse, reddish-orange halo. The overall structure suggests a spiral or lenticular type, with a possible disk structure. However, irregularities or subtle disturbances are present in the outer regions, which may be indicative of past or ongoing interaction with another galaxy. The galaxy is roughly symmetrical overall, with some signs of asymmetric features or tidal tails visible.
