The galaxy presents as a disk-shaped structure, viewed nearly edge-on. The central region displays a bright, concentrated bulge, potentially indicating an older stellar population. The color gradient suggests a possible increase in blue light from the outer disk, inferring the presence of younger, star-forming regions. The lack of easily discernible spiral arms and overall smooth appearance hints at a galaxy with a well-defined disk component. The lack of dust lanes along the edge-on disk is also notable. Based on its morphology, this galaxy is likely to be a spiral galaxy with a significant bulge, seen from an angle close to edge-on.
