The galaxy appears as a luminous, elliptical-shaped object with a smooth, diffuse morphology. The central region exhibits a high surface brightness, appearing almost uniformly bright and gradually decreasing in intensity towards the outer edges. The color profile suggests a slightly redder hue in the central bulge, indicative of an older stellar population, while the outer regions appear somewhat bluer. No distinct spiral arm structures or dust lanes are visible within the galaxy's structure; it presents a generally featureless, spheroidal appearance. There is a slight asymmetry in the outer halo, suggesting possible gravitational interactions, although no major tidal disturbances are readily apparent. The overall roundness of the structure suggests a classification towards the earlier types of galaxies.
