The galaxy appears to be a relatively smooth, disk-shaped object, viewed at an oblique angle. The central bulge is prominent and has a yellowish hue, suggesting an older stellar population. The disk itself exhibits a bluer tint, possibly indicating the presence of younger, hotter stars. There is a slight elongation to the galaxy's shape, but it does not appear to be highly elongated, indicating the object is somewhat round. No distinct spiral arms or prominent dust lanes are readily visible within the disk. There is no evidence of major tidal disturbances or ongoing mergers. The overall structure suggests a galaxy that has largely settled into a relatively quiescent state, with minimal signs of recent major star formation events.
