The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its overall color is yellowish-orange, suggesting a population of older stars with lower rates of recent star formation. There is a bright central bulge, which gradually fades into the outer regions of the galaxy. The galaxy exhibits a fairly regular, round shape with no visible spiral arms or significant dust lanes. There is no evident tidal disruption or nearby merging companions, indicating that it may be a relatively isolated system. Its structure appears mostly undisturbed, without significant asymmetries or morphological peculiarities.