The galaxy presents a largely smooth and rounded morphology. A concentrated central bulge exhibits a yellow-orange hue, indicative of an older stellar population with lower ongoing star formation. A fainter, diffuse disk is observed surrounding the bulge. There is no apparent spiral structure. The galaxy appears relatively undisturbed, showing little evidence of recent major mergers. There may be some slight tidal features indicative of a minor past disturbance. Overall the galaxy shows that it is a relatively high mass object.
