The galaxy appears as a single, luminous object. It exhibits a relatively smooth and featureless morphology, with a dominant spheroidal component. The galaxy's shape is generally round. There is no strong indication of spiral arms or a prominent disk.

The color gradient suggests a high density of older stellar populations. The galaxy does not present any strong evidence of active star formation. There are no indications of major disturbances or merging events, and the system seems relatively isolated.
