The galaxy presents as a moderately bright, elliptical-like structure. The core appears luminous and relatively uniform, with a yellow-white hue suggesting an older stellar population. There is a slight elongation observed, indicating it is not perfectly spherical, but it is still mostly round in appearance. A possible merging event may be occurring as there is a large, but faint, red area on the edge of the galaxy. Based on the overall smooth light distribution, it is unlikely to have strong spiral arm features. There appear to be minimal signs of active star formation within the core. The galaxy does not appear to be severely disturbed.
