The galaxy appears as a somewhat rounded, centrally concentrated object with an overall smooth morphology. There is evidence of a potential merger event occurring. One distinct, compact region of enhanced red emission is separated above the primary body. This could possibly suggest ongoing star formation. The primary body presents a bright, centralized core fading into the outer regions with more diffuse blue and green colors, suggestive of a spiral shape. The bulk of the galaxy appears to be relatively undisturbed, with only minor distortions to its overall shape.
