The galaxy presents a generally smooth, elliptical morphology. The light profile is centrally concentrated, with a gradual decrease in intensity outwards from the core. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population, with less recent star formation. While the structure is largely smooth, there is a slight asymmetry, possibly indicating a minor gravitational interaction or disturbance. There is a slight disk appearance. No spiral arm structures are discernible in the image resolution. The overall form is generally rounded, although it is difficult to completely resolve from the image provided. 
