The galaxy presents a largely smooth, elliptical morphology. It appears highly spheroidal in shape, exhibiting a high degree of circularity. The color profile suggests a dominant population of older stars, with a yellowish-red hue concentrated towards the center. There is little evidence of distinct spiral arms or prominent dust lanes, suggesting the absence of significant ongoing star formation. The galaxy shows a central brightening, likely indicating a concentration of stars towards the galactic nucleus. Overall, the galaxy exhibits characteristics consistent with a mature, quiescent elliptical galaxy. Minor asymmetry might be present, suggesting possible recent minor interactions, however the galaxy appears to be mostly undisturbed.
