The galaxy appears as a somewhat diffuse object, exhibiting a slight elongation suggesting a possible disk-like structure viewed at an angle. The central region is brighter and more concentrated, possibly indicating the presence of a galactic bulge or nucleus. Moving outward from the core, the light distribution becomes more irregular and patchy. There are hints of spiral arm structures or other features in the outer regions of the galaxy. The overall color is a mix, with bluer hues mixed within. This color variation suggests that the galaxy may contain mixed stellar populations. Patches of bluer light hint at recent star formation events. There is a possibility of tidal tails or a minor merger event affecting the overall shape. 
