The galaxy appears as a moderately bright, elliptical object with a smooth, diffuse light distribution. Its core exhibits a concentrated brightness, transitioning gradually outward to a less luminous halo. There is little evidence of spiral arms or distinct substructure, the overall form appearing relatively homogenous. The color profile suggests a population of older stars dominating the galaxy, giving it a reddish-yellow hue, while a subtle greenish tint in the outer regions might indicate the presence of some younger stars or ionized gas, although this is less prominent. The galaxy's apparent shape is slightly elongated, and there are no clear signs of ongoing major mergers or significant tidal disturbances based on the overall symmetry and lack of highly distorted features.
