The galaxy presents as a predominantly smooth, elliptical-like object, exhibiting a high degree of central concentration. The core region displays a bright, yellow hue, possibly indicating an older stellar population. The light from the galaxy is generally smooth, but some regions exhibit a slightly bluer coloration. There is no evidence of spiral arms or a prominent disk structure and the galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances. Overall, this galaxy appears to be a well-formed elliptical galaxy with an old stellar population.
