The galaxy presents as a relatively smooth and centrally concentrated object, appearing elliptical in shape. There is a clear central bulge with a yellowish-red hue, suggesting an older stellar population dominates this region. The outer regions of the galaxy exhibit a bluer tint, possibly indicating some ongoing star formation or a younger stellar population at the periphery. There may be minor gravitational disturbances visible, as the morphology shows a slight asymmetry or warping.
