The galaxy exhibits a roughly elliptical morphology, appearing relatively compact and centrally concentrated. The core region presents a bright, slightly elongated structure. There's evidence of a disk-like component extending from the central bulge. The color gradient across the galaxy indicates a change in stellar populations and dust distribution, with bluer colors concentrated in the central regions and redder tones towards the outer edges, suggestive of ongoing or recent star formation in the core. No spiral arm structures or significant tidal features are obviously visible, though there is evidence of minor disturbance/merging occuring. 
