The galaxy presents as a predominantly smooth, elliptical structure. Its overall form is moderately rounded, transitioning smoothly from a bright, concentrated central bulge to a more diffuse halo. The core exhibits a yellowish hue, suggesting an older stellar population, while the outer regions display a slightly bluer tint, hinting at the presence of some younger stars, although star formation appears to be subdued. There are subtle irregularities in the outer halo that might indicate a past or ongoing minor interaction. The galaxy shows no prominent spiral arms or a well-defined disk. 
