The galaxy presents as a slightly elongated, elliptical-like structure with a smooth, diffuse light distribution. It exhibits a concentrated central bulge that gradually fades into the outer regions. The color profile suggests a population of older stars, with a yellowish hue dominating the overall appearance. There is a faint hint of a disk-like structure, but the galaxy is mostly devoid of prominent spiral arms or distinct features. No significant dust lanes or regions of active star formation are readily apparent. The overall morphology indicates a relatively evolved galaxy.
