The galaxy presents a centrally concentrated morphology. The core region exhibits a bright, diffuse glow that fades gradually outwards. The overall form leans toward elliptical, though there are hints of a disklike structure, potentially indicating a spiral galaxy viewed at an angle. Within the extended halo, there are structural irregularities that suggest possible tidal disturbances or ongoing mergers. The color profile shows a slightly bluer tint in the outer regions, possibly suggesting more recent star formation activity away from the central bulge. The central region exhibits a more red-shifted color, indicating an older stellar population. A slight deviation from perfect roundness is noticeable, with a suggestion of some internal structure. Overall, the galaxy appears to be a relatively massive system undergoing some form of interaction or disturbance.
