The galaxy presents as a somewhat flattened, disk-like structure, appearing elongated with a cigar-shaped morphology. The central region exhibits a smoother texture and is visually brighter with a slightly bluish tint, suggesting a concentration of younger stars or possible active galactic nucleus activity. The galaxy seems relatively isolated, with some hint of a minor asymmetry or disturbance in its structure, possibly indicating past or ongoing interaction with a smaller companion galaxy or gravitational disruption. The outer regions are fainter, gradually fading into the background sky. Overall, the galaxy appears to be a spiral or lenticular type with a relatively small mass.
