The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. The light distribution suggests a primarily spheroidal structure, with little evidence of a disk component or spiral arms. The galaxy exhibits a yellowish-red hue, which indicates an older stellar population and relatively low ongoing star formation. There is a slight asymmetry in the galaxy's light profile, possibly indicating a minor interaction or disturbance. Overall, it appears to be a fairly relaxed, evolved system.
