The galaxy presents as a somewhat smooth, elongated structure. The central bulge exhibits a concentrated luminosity gradient, appearing significantly brighter and more yellow-orange than the outer regions. The disk component is visible, though relatively ill-defined, extending outward from the bulge. The disk color appears more blueish-green relative to the bulge. The overall morphology suggests a galaxy somewhere between a pure elliptical and a spiral, possibly a lenticular galaxy, viewed at a significant angle, closer to edge-on. There are no obvious signs of active merging or major disturbances in the galaxy's morphology, although subtle irregularities in the disk cannot be ruled out.
