The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated, bright central region, likely a bulge component. A gradual fading of luminosity occurs outwards from the center, indicating a decrease in stellar density. The galaxy appears generally featureless with no distinct spiral arms or bar structure visible. The color profile is relatively uniform, with a slight bluer hue in the outer regions suggesting the presence of a younger stellar population or some minor star formation, although at a low rate. There is no obvious indication of tidal disturbances or ongoing mergers, and the galaxy appears relatively isolated and undisturbed.
