The galaxy presents as a moderately faint, elongated, and somewhat disturbed system. The primary structure appears to be a disk galaxy, viewed at a high inclination. The central region exhibits a brighter, slightly diffuse glow, suggesting a potential bulge or a concentration of older stellar populations.

The disk component shows evidence of some structure, although precise arm morphology is difficult to discern. There are hints of patchy, bluer regions scattered throughout the disk, potentially indicative of ongoing star formation within HII regions. The overall color is blue, implying a younger stellar population.

The galaxy exhibits a slight asymmetry, which could be due to a recent minor merger event or tidal interactions. There are no obvious signs of strong tidal tails, but a subtle disturbance in the disk's outer regions may suggest gravitational interaction. The galaxy appears to be relatively isolated, without any obvious nearby companions, except for the foreground objects.
