The galaxy presents as a somewhat amorphous, though generally rounded, structure. The central region exhibits a notably concentrated luminosity, appearing a yellow-white hue suggesting an older stellar population. Moving outward from this central core, the light gradually diminishes, transitioning into fainter, less defined outer regions. There is a possible indication of spiral arm remnants or tidal features appearing blue, particularly extending in a slightly disturbed manner from the main body of the galaxy. These features are somewhat diffuse and do not present a highly organized or well-defined spiral structure. The galaxy lacks the sharp, distinct edges characteristic of some spiral galaxies, suggesting a more elliptical nature or a galaxy undergoing some form of interaction or disturbance.
