The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. There is a subtle color gradient, shifting from a more yellowish central region to a bluer periphery. No distinct spiral arms or bar structures are discernible. The overall light distribution suggests an older stellar population. Faint disturbances or tidal features may be present, though they are subtle, which could possibly be indicative of a past or ongoing minor interaction or merger event, yet the dominant impression is that of an evolved system. The galaxy's roundness indicates that is either a face-on spiral or an elliptical galaxy. There is little active star formation.
