The galaxy presents a morphology that leans towards a smooth, relatively featureless structure. Its overall shape appears elliptical, with a notable absence of prominent spiral arms or a well-defined disk. There is some evidence of subtle irregularities or minor disturbances in its outer regions, potentially indicative of past interactions or ongoing accretion events. The galaxy displays a color gradient, appearing somewhat bluer in its central region and gradually becoming redder towards the outer edges. This color variation suggests a younger stellar population concentrated in the core, with older, redder stars dominating the outskirts. The galaxy is moderately luminous, emitting a significant amount of light across the observed bands. Its size is appreciable, spanning a considerable angular extent in the image. The lack of substantial dust lanes or prominent star-forming regions further supports its classification as an elliptical galaxy, likely residing in a more evolved state with a relatively low star formation rate.