The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. It exhibits a subtle elongation, appearing somewhat cigar-shaped. The color profile suggests an older stellar population, with a yellowish hue dominating the core region, potentially indicative of evolved stars. There's little evidence of active star formation in the visible spectrum, as the color is largely devoid of the blue or intense red associated with HII regions. No obvious spiral arm structures or dust lanes are discernible. The overall morphology points toward a galaxy that has largely completed its major mergers, displaying a relaxed, quiescent state.
