The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellow-orange hue, suggestive of an older stellar population with minimal ongoing star formation. There is a subtle, almost imperceptible, disk-like structure, yet the light is dominated by the bulge. The galaxy shows no strong signs of tidal disturbances or major mergers, although a possible minor asymmetry in its outer regions could indicate past interaction. It presents a moderate degree of ellipticity, appearing slightly elongated rather than perfectly spherical. The galaxy's core is bright and well-defined, indicating a concentrated central region.
