The galaxy presents as a moderately bright, face-on system. Its overall morphology is elliptical with a central, intensely luminous core, suggestive of an active galactic nucleus or a significant concentration of older stars. The outer regions of the galaxy exhibit a diffuse halo. There's a slight irregularity in the smooth distribution of light, hinting at possible minor interactions or internal disturbances. The color profile indicates a mixed stellar population, with a dominant yellow-red component. The lack of distinct spiral arms or prominent dust lanes suggests a relatively passive star formation history.
