The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial color gradient, transitioning from a yellowish core to a redder outer halo. There is little evidence of significant spiral arm structure or prominent dust lanes. The galaxy appears relatively undisturbed, lacking clear signs of ongoing major merger activity, though a faint, subtle asymmetry in the outer regions might indicate a past minor interaction. Overall, the galaxy suggests a mature stellar population with suppressed star formation.
