The object presents as a singular galactic entity with a smooth, consolidated morphology. There are two primary light concentrations. The brighter region exhibits a yellow-orange hue, suggesting a population of older stars. A secondary, less intense, concentration displays a yellower tone, potentially representing a distinct stellar population or region of differing age. The overall form is generally round. Some apparent disruption within the galaxy could be interpreted as signs of minor disturbances. The galaxy exhibits colours consistent with an elliptical galaxy with moderate star formation activity.
