The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. There is little evidence of spiral arms or a prominent disk component. The galaxy exhibits a yellowish-orange hue, potentially indicating an older stellar population with lower rates of on-going star formation. There may be a slight flattening along one axis, but it primarily appears quite round. There are no obvious signs of tidal disturbances or a major merger event.
