The galaxy presents a generally smooth morphology, with a near-spherical, moderately concentrated light distribution. The central region exhibits a distinct reddish-orange hue, which appears to fade into a less saturated yellowish color towards the outer regions. There are no apparent spiral arms or distinct features indicative of ongoing major mergers or disturbances. The overall color profile suggests an older stellar population, with potential for a low rate of star formation. The galaxy exhibits a centrally concentrated bulge that appears nearly round, and a smoother profile indicative of an elliptical classification.
