The galaxy appears as a generally smooth and rounded structure, with a slightly concentrated central region suggesting the presence of a bulge. There is a subtle color gradient, trending from a more yellowish hue at the core to a slightly bluer tinge in the outer regions. No distinct spiral arms or bar structures are discernible. There is no apparent indication of any major ongoing merger events or strong tidal distortions. The overall morphology indicates a relatively evolved galaxy. The absence of prominent star-forming regions supports the inference of a relatively low star formation rate.
