The galaxy presents a generally smooth and elliptical morphology, exhibiting a highly concentrated central bulge. The color profile suggests an older stellar population, with a yellow-orange hue dominating the visible light. There is no clear evidence of spiral arms or prominent dust lanes. The galaxy appears relatively undisturbed, with no major tidal features or signs of ongoing mergers. A slight elongation is present, with a generally round overall appearance. Star formation appears to be minimal within the galaxy.
