The galaxy presents as an elliptical morphology, with a smooth, concentrated luminosity profile. The central region exhibits a yellowish-white hue, suggesting an older stellar population. There is a noticeable, though subtle, decrease in luminosity with radial distance from the center, indicating a relatively quiescent galaxy with minimal ongoing star formation. Its overall shape is moderately elliptical, appearing neither perfectly spherical nor highly elongated. Faint hints of a slight disturbance or asymmetry can be observed at the periphery, but it mainly looks like a relatively isolated galaxy.
