The galaxy presents as a roughly elliptical structure with a dominant central bulge. It exhibits a smooth light distribution, suggesting a lack of significant spiral arm structures. The core is intensely bright, transitioning to a slightly fainter halo. The color profile indicates a redder hue, especially in the central regions, implying an older stellar population. A slight asymmetry or subtle disturbance is visible, with a faint elongation or possible tidal feature extending outward.
