The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a moderate degree of ellipticity, appearing somewhere between round and elongated. No distinct spiral arms or bar structures are discernible within the limits of the image resolution. The galaxy core appears bright and diffuse, suggesting a significant concentration of stars in the central region. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy displays a colour gradient, becoming bluer towards the outer regions. This colour likely indicates that the stars are mainly older, but there is also a good deal of younger, bluer stars in the outer regions.