The galaxy presents as a relatively smooth and centrally concentrated object. The light profile indicates a bulge-dominated system, with a slight elongation or asymmetry suggesting a possible disk component or a minor interaction. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer emissions are seen, possibly suggesting areas of ongoing star formation. Overall, the galaxy appears relatively undisturbed, but there might be minor disturbances occurring.
