The galaxy presents a largely smooth, elliptical morphology. Its core is a bright, concentrated source of light, exhibiting a yellowish-orange hue, suggestive of an older stellar population and minimal ongoing star formation. There is a slight elongation, though the galaxy appears generally round. A faint halo of light surrounds the central region, indicating the presence of a diffuse stellar component extending beyond the core. The galaxy appears relatively isolated, showing no obvious signs of tidal disturbances or interactions with other galaxies, although there are a couple of close neighboring objects to the lower-left. These do not appear to be disturbing the galaxy.
