The galaxy appears as a slightly elongated, yellowish-orange elliptical galaxy. It has a high degree of central concentration, with the light intensity diminishing smoothly outward from a bright core. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a smooth, featureless morphology, suggesting an older stellar population. The light profile indicates a shape leaning towards "in between" round and cigar-shaped, rather than perfectly spherical or highly elongated. There is no apparent major disturbance or ongoing merger activity. The galaxy seems relatively isolated, without obvious signs of interaction with nearby galaxies.
