The galaxy presents a somewhat elongated, disk-like morphology, likely viewed at an oblique angle, but not quite edge-on. A central bulge is visible with a yellow-ish hue, potentially indicating an older stellar population. Extending outward from this central region are fainter, more diffuse disk components. Hints of bluer regions are observable, which could represent regions of more recent star formation. The overall structure appears relatively undisturbed, though slight irregularities might suggest minor gravitational interactions.
