The galaxy presents as a centrally concentrated, smooth, elliptical-like structure. It exhibits a moderate degree of roundness. There is no evidence of prominent spiral arms or a well-defined disk component. The galaxy appears to be dominated by an older stellar population, with a yellowish-white hue indicating a lack of significant ongoing star formation. There might be a slight hint of asymmetry in the outer regions, possibly indicative of a past minor interaction or disturbance, but the overall structure remains largely undisturbed. The galaxy shows a clear central bulge that blends smoothly into the surrounding halo.
