The galaxy presents as a relatively compact object with a smooth, elliptical morphology. A slight elongation is visible, though it is mostly round. The central region exhibits a concentration of light, suggesting a bulge. Faint features are present, with potential minor disturbances in its overall structure. The galaxy displays a reddish hue, indicating a population of older stars and a low rate of ongoing star formation. There might be an ongoing merger event causing the disturbance.