The galaxy presents as a single, relatively smooth object. Its overall morphology appears elliptical, trending toward moderately rounded, with little discernible fine structure or distinct features such as spiral arms or a prominent disk. The light profile exhibits a concentrated, bright central region, likely the galactic nucleus, which gradually fades into a more diffuse halo. The color distribution suggests an older stellar population. The galaxy appears isolated and undisturbed with no indication of active merging events.
