The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a bright, concentrated core that gradually diffuses outwards. The overall shape is somewhat rounded. The color profile suggests a mix of stellar populations, with a slightly bluer hue in the outer regions transitioning to a redder tint in the core. No distinct spiral arms or bar structures are readily apparent. There are no obvious signs of a major ongoing merger, though subtle asymmetries in the outer envelope might indicate minor tidal interactions or past disturbances.
