The galaxy presents an elliptical morphology, appearing largely smooth with a slight elongation. There is a marginal asymmetry in its structure, though no clear indication of recent major merger activity. The galaxy's light distribution suggests a concentration of older stellar populations, with subtle color variations throughout its body. Star formation activity appears to be relatively low. Based on its structure and color profile, this is likely an evolved galaxy with moderate mass. There is no clear indication of a strong disk component, and the overall appearance is consistent with a relaxed system.
