The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bright core, which gradually diffuses outwards into a less luminous halo. There is a slight elongation observed, moving away from a circular shape. Faint blue tinges appear within the central region of the galaxy. No strong evidence of prominent spiral arms, dust lanes, or significant tidal disturbances is observed, indicating the galaxy is not actively merging. Overall, it seems to be a fairly undisturbed galaxy.
