The galaxy presents a largely smooth morphology with a centrally concentrated light profile. The overall shape is close to round. There is a subtle suggestion of a disk component, but it is not well-defined. Evident are possible signs of minor disturbances in its structure. It exhibits a color gradient, appearing bluer towards the outer regions and redder towards the center, possibly indicating a younger stellar population in the outer regions. No prominent spiral arms or a well-defined bar structure are visible. The galaxy appears relatively isolated, without obvious signs of ongoing major mergers, though there is evidence to suggest past interaction events.
