The galaxy presents an overall smooth, elliptical morphology with a centrally concentrated bulge. The light distribution is relatively uniform, suggesting an older stellar population and low star formation rate. The color gradients indicate a redder core, transitioning to bluer hues in the outer regions. There is no apparent spiral structure or distinct dust lanes, and the overall appearance is consistent with that of an early-type galaxy, potentially an elliptical or lenticular. Faint tidal features may be present, warranting further investigation to confirm the likelihood of a recent or ongoing minor merger event. The galaxy appears roughly circular. The redder color of the core suggests that it is composed of older stars. 
