The galaxy presents as a luminous, generally elliptical object. It exhibits a smooth, centrally concentrated morphology with a radial profile that gradually decreases in intensity outward from the core. The color profile appears relatively uniform across the visible spectrum, suggesting a somewhat homogenous stellar population. There is a slight elongation visible but overall it exhibits a circular shape. No distinct spiral arm structures, dust lanes, or prominent star-forming regions are readily discernible. No obvious signs of tidal interactions or recent merger events can be confirmed.
