The galaxy presents an overall asymmetrical morphology, appearing disturbed. It shows a prominent, moderately sized bulge with a diffuse outer region. Evidence of a possible interaction or merger is observed, with what appears to be a smaller object in close proximity to the main galactic body. The tidal disturbances seem more akin to a merger than a tidal interaction. There appears to be significant star formation occurring within the galaxy, as evidenced by the apparent blue tint in the outer regions, although this could also be due to disturbances. The bulge exhibits a yellower color, indicative of an older stellar population. It cannot be conclusively determined if the galaxy is barred or contains spiral arms due to the apparent disturbances and the limited resolution of the image, though there may be evidence of weak bar structure. 
