The galaxy presents as a generally smooth object with a moderately elliptical morphology. The light distribution suggests a bulge-dominated system with a somewhat diffuse outer halo. There is a subtle color gradient visible, transitioning from a central yellowish hue to a slightly bluer tint at the periphery. No distinct spiral arm structures are discernible. There is an apparent lack of major tidal disturbances or indications of ongoing or recent major merger activity. The galaxy appears relatively isolated, and the overall impression is that of a relatively quiescent system.
