The galaxy presents a smooth, elliptical morphology with a relatively high degree of central concentration. The light distribution suggests a centrally dominant bulge, which may indicate an older stellar population within the galactic core. There is a subtle color gradient from the core outwards, with the central region appearing slightly more yellowish. The faint outer regions imply a lower surface brightness envelope extending outwards. While there are some very subtle hints of possible disturbances or faint tidal features in the surrounding region, the overall impression is that of a largely undisturbed system. The galaxy is approximately round, displaying very little flattening. There are no clearly identifiable spiral arms or distinct disk features visible.
