The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a distinct yellowish-gold hue, potentially indicating an older stellar population. The light profile diffuses outwards from the core, fading into a less structured halo. There is little to no apparent evidence of spiral arms, a distinct disk, or significant dust lanes. The overall appearance suggests a lack of recent major merger activity. Subtle disturbances may exist in the outer regions, though these are faint. The galaxy is relatively compact and appears to be one singular object.
