The observed galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, showing a slight deviation from perfect circularity. The color profile suggests a redder core transitioning to somewhat bluer outer regions. While a predominantly smooth structure is apparent, there is a hint of minor disturbances in the outer regions, which could be indicative of ongoing or past interactions. There is no clear sign of a prominent disk structure or major mergers. Overall, the galaxy presents as a largely undisturbed system with a smooth light distribution.
