The galaxy presents as a relatively smooth, rounded structure. A bright, concentrated central region, potentially indicative of a galactic nucleus, is visible. The light distribution suggests minimal features or a disk-like structure, with a lack of distinct spiral arms or prominent dust lanes. The galaxy exhibits a slight color gradient, transitioning from a yellowish-white core to a bluish outer halo. There is no obvious evidence of ongoing major mergers or tidal disturbances, though a very subtle asymmetry may indicate minor interactions.
