The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology is elliptical or lenticular. The central bulge is prominent and appears yellowish-white, suggesting an older stellar population with fewer young, massive stars. Moving outward from the core, the light fades gradually. There is a subtle blue tinge, possibly indicative of ongoing, though limited, star formation within its disk or halo. There appears to be a very slight asymmetry in the outer regions, but it is not significant enough to suggest a major ongoing merger event. The galaxy seems to be generally undisturbed.
