The galaxy presents as a largely elliptical morphology, displaying a smooth, concentrated central bulge. The galaxy exhibits a dominant orange-yellow hue throughout the central region, suggesting an older stellar population. Fainter blue-green emissions are observed in the outer regions indicating relatively small amounts of ongoing star formation or the presence of younger stellar populations. There is no clear spiral arm structure visible. The galaxy appears mostly undisturbed, exhibiting no strong tidal features or signs of a recent major merger. The shape appears to be consistently elliptical in nature, displaying a slight ellipticity as opposed to a perfect circle.
