The galaxy presents as a somewhat elliptical, disk-like structure when viewed from this angle. The central bulge is prominent and appears relatively smooth. Moving outward from the center, the disk becomes less distinct, with some faint features, but no clear spiral arm structure is discernible. There is a slight color gradient from the center outward; the core region is a warmer tone than the disk, indicating potentially older stellar populations. The disk appears to have some dust lane absorption or regions of ongoing star formation. The galaxy's overall shape is not perfectly regular. The slight distortions potentially point towards minor gravitational interactions or internal activity that is disrupting its morphology.
