The galaxy appears as a late-type spiral galaxy, presenting an almost edge-on orientation relative to our line of sight. The disk structure is clearly visible, bisecting the galaxy into two symmetrical halves. There is a subtle central bulge, elongated along the disk axis, with a rounded morphology. The galaxy exhibits a relatively smooth disk, with limited visible evidence of strong spiral arm structures or prominent star-forming regions. The color suggests a mix of stellar populations, with a tendency towards older, redder stars dominating the visible light. There is no indication of ongoing major merging events or significant tidal disturbances in the immediate vicinity of the galaxy.
