This galaxy presents a predominantly smooth morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar density. Moving outwards from the core, the luminosity gradually decreases. There's evidence of a faint, extended disk structure, hinted at by the subtle color variations around the central bulge. The galaxy appears somewhat elliptical, with an intermediate axial ratio, leaning towards a more rounded shape rather than a highly elongated one. No prominent spiral arms or significant dust lanes are visible. There are only very minor visual disturbances or signs of ongoing merger activity. The overall color profile indicates a population of older stars. The reddish hue is observed in the central bulge, gradually transitioning to slightly bluer shades in the outer regions of the galaxy. This color gradient could indicate differences in stellar populations or variations in the rate of recent star formation activity across the galaxy. 
