The galaxy presents as a centrally concentrated, luminous object with a relatively smooth morphology. It is observed to have a generally elliptical shape with a high degree of roundness. The core region is particularly bright, displaying a gradual decline in surface brightness towards its outer regions. A faint, diffuse halo surrounds the central body of the galaxy. There is very little evidence of prominent disk-like structures or spiral arms. The overall color appears relatively uniform, suggestive of a fairly homogenous stellar population. Subtle irregularities in the outer halo may indicate minor gravitational interactions or disturbances. There does not appear to be a significant ongoing merger event.