The galaxy presents as a largely elliptical structure, with a smooth, diffuse light profile concentrated towards the center. There is a subtle elongation, suggesting a departure from perfect sphericity. The primary color component is a yellowish-orange hue, likely indicative of an older stellar population and minimal ongoing star formation. Faint, diffuse bluer regions are sparsely distributed in the outer regions of the galaxy. There is possibly a minor tidal disturbance or interaction with a smaller galaxy located nearby.
