The galaxy presents as an elliptical morphology with a dominant central bulge. The light distribution appears relatively smooth, suggesting a well-mixed stellar population. There's a noticeable color gradient from the core outward, transitioning from a yellow/gold center towards redder hues in the outer regions. This reddening could be indicative of older stellar populations or increased dust obscuration at larger radii. No obvious spiral arm structures or prominent dust lanes are visible. The overall symmetry indicates a system that is not currently undergoing major merger activity, though minor disturbances cannot be ruled out. There appears to be a faint extended halo of light surrounding the main body of the galaxy.