This galaxy exhibits a predominantly smooth morphology with a likely disk component. The central bulge is bright and concentrated, with a relatively diffuse halo extending outwards. The galaxy appears to be somewhat flattened, leaning towards a more elliptical shape rather than a perfect sphere. There is a hint of bluer colors, possibly indicative of ongoing star formation. Some minor distortions or disturbances in its overall structure are present. This suggests a possible recent interaction or merger. The majority of the structure is contained within the inner regions, with the outer edges fading into the background.
