The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy transitions into a fainter, more diffuse halo. The overall shape is more elliptical than disk-like. There is minimal evidence of spiral arm structures or significant dust lanes within the galaxy. There are no signs of active merging, with a fairly relaxed, undisturbed morphology. Faint, blueish tinges within the outer regions could indicate more recent star formation, though this is not prominent. Overall, this galaxy appears to be a mature system with ongoing, but minimal star formation.
