This galaxy presents as a somewhat elongated, lenticular structure with a smooth, concentrated central bulge. The light distribution suggests a fairly symmetrical shape, with the isophotes appearing flattened along one axis. The color profile transitions from a bluer hue at the edges to a more yellow-red central region, possibly indicating older stellar populations towards the core and younger populations in the outer regions. There is no clear evidence of spiral arms or active star formation regions visible in this image. The galaxy shows no obvious signs of major disturbances or ongoing mergers.