This galaxy appears to be a luminous, relatively smooth, and compact system. It exhibits a centrally concentrated brightness profile, with a yellowish hue suggesting a population dominated by older stars. While the galaxy appears mostly smooth, there is a hint of a disturbed morphology or potential tidal features extending from the central region. The shape is generally round. There is also a significant chance that the galaxy is merging with another galaxy. The system may have a low star formation rate.
