The galaxy presents as a yellowish, moderately luminous object with a somewhat elliptical morphology. The light is centrally concentrated, diminishing gradually toward the outer edges without exhibiting distinct spiral arm structures or a prominent disk. The overall appearance is smooth, lacking clear signs of significant ongoing star formation or substantial dust lanes. There is a slight asymmetry in the outer regions, hinting at possible past or ongoing minor interactions, but the system appears generally undisturbed. The color suggests a relatively older stellar population.
