The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge, transitioning to a more diffuse outer region. The color profile indicates a yellowish-white hue at the core, possibly indicative of an older stellar population. A slight color gradient towards the outer regions may suggest subtle differences in stellar age or composition. There is no apparent spiral structure or distinct dust lanes. Overall, the galaxy appears as a relatively undisturbed, early-type galaxy, likely elliptical or lenticular in nature. There may be some subtle signs of minor disturbances.
