The galaxy appears to be an elliptical or lenticular type. It exhibits a largely smooth and centralized light distribution with a high degree of radial symmetry. The central region has a high concentration of light, appearing nearly spherical with a slightly elongated shape. The color of the central bulge appears yellowish-white suggesting an older stellar population. A faint, diffuse disk-like structure is faintly visible, extending outward from the central bulge. There are noticeable asymmetries and disturbances in the outer regions of the galaxy, particularly on the left side, potentially indicating interactions or recent mergers. These disturbances manifest as irregularities in the light distribution. Faint tidal features and signs of ongoing interactions are present, further implying the possibility of past or ongoing mergers or interactions with other galaxies.
