The galaxy presents a predominantly smooth morphology with a central bulge. The galaxy appears to be disk-like and without a barred structure. There is a lack of prominent spiral arms or distinct star-forming regions visible within the galaxy's disk. The galaxy appears to be undergoing minor gravitational disturbance. The galaxy exhibits a color gradient, transitioning from a bluish hue in the core to a redder tint towards the outer regions. This may indicate an older stellar population residing in the outer regions with ongoing star formation in the central regions. The overall appearance suggests a system with relatively low levels of recent star formation.
