The galaxy presents as a somewhat elongated, disk-like structure, seen at an oblique angle. It exhibits a central, bright, yellowish bulge that dominates the galaxy's overall luminosity. The outer regions of the disk show a bluer hue, suggesting the presence of younger stellar populations and possibly ongoing star formation. Faint, diffuse features or structures might be present in the disk, but are difficult to resolve clearly. The overall appearance suggests a relatively undisturbed morphology, lacking signs of major mergers or tidal disruptions. The galaxy appears to be a fairly massive system, with moderate levels of star formation relative to its stellar mass.
