The galaxy appears as a single, luminous structure with a generally elliptical morphology. The light distribution is concentrated towards the center, with a smooth gradient outwards, indicating a likely lack of significant spiral arm structures or distinct features. The core exhibits a bright, unresolved nucleus. Overall coloration suggests a population of older stars, which typically presents as a yellow or reddish hue, but the presence of some bluer regions may imply some recent star formation as well. The galaxy appears to be undergoing a merger or tidal interaction as there appears to be a smaller system interacting with the primary object, deforming it slightly. The overall size is relatively compact.
