The galaxy presents a faint, somewhat diffuse appearance. The color profile seems to indicate a mixed stellar population, with a slight concentration of redder hues in what could be the galactic bulge or core. A hint of a spiral arm structure might be present but appears significantly disturbed or irregular. The galaxy exhibits no definitive central point and appears elongated rather than spherical, with the possible hint of tidal features or distortions. Overall, the morphology leans towards a disturbed or potentially merging system, with a small possibility of minor interaction evident in the diffuse features and color variations across the galaxy's body. High artifact probability.
