The galaxy presents a generally smooth, elliptical morphology with a dominant central bulge. Its shape appears to be closer to in between rounded and elliptical. There are no strongly defined spiral arms visible; instead, the light distribution is more diffuse. The core of the galaxy exhibits a concentrated, brighter, yellowish-white hue, suggesting an older stellar population. The outer regions show a fainter, bluer tint. The lack of obvious tidal tails or dramatic distortions suggest a quiescent state, though a minor disturbance or interaction cannot be entirely ruled out.
