The galaxy presents as a largely amorphous, elliptical shape with a smooth overall appearance. There is no clear disk structure visible, but a slight elongation is discernable. The central region appears brighter and more concentrated, likely indicating a dense nucleus or bulge. Color gradients are subtle but present. The core exhibits a brighter, bluer hue transitioning to a more yellow and red tint towards the outer regions. Given the lack of spiral arms or prominent dust lanes, the galaxy appears to be a relatively evolved system with little ongoing major star formation activity. Possible minor interaction or internal disturbance is subtly indicated.