The galaxy presents as a somewhat flattened elliptical or lenticular system. It exhibits a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population. A diffuse disk extends outwards from the bulge, displaying a bluer hue, possibly indicating more recent star formation. The disk appears relatively smooth, lacking prominent spiral arm structures or distinct dust lanes. Overall, the galaxy demonstrates a relatively high degree of symmetry and no obvious signs of ongoing major mergers or significant tidal disturbances, although there might be minor disturbances. The light distribution suggests that the galaxy is relatively massive and has experienced a complex history of star formation, with a dominant older population and ongoing activity within its disk.
