The galaxy appears as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. It exhibits a prominent central bulge which is yellowish-white in color, indicating an older stellar population. The outer regions are characterized by a bluish halo, suggesting the presence of younger, hotter stars and ongoing star formation, although at a low rate. There is some evidence of minor disturbances or asymmetries in the outer regions, potentially hinting at a past interaction or merger event, but these are not dramatically disruptive to the overall structure. The galaxy lacks any clearly defined spiral arm structure.
