The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in form. The central region exhibits a bright, luminous core, indicating a high concentration of stars and potentially an active galactic nucleus. A faint reddish halo surrounds the central core, which then fades into the surrounding darkness. The outer regions show slight disturbances, perhaps from smaller galactic interactions. The overall color profile suggests an older stellar population, with minimal evidence of active star formation in the main body of the galaxy.
