The galaxy exhibits a flattened, elongated morphology suggestive of a disk galaxy viewed at an oblique angle. The light distribution appears relatively smooth, with a gradual decline in surface brightness from the center outwards. There is a subtle suggestion of a central bulge, although the image resolution is limited. The colors are generally consistent across the galaxy, indicating a relatively uniform stellar population, but there may be slight color variations. There is no obvious strong spiral arm structure or prominent dust lanes visible, nor is there a large tidal disturbance. A subtle asymmetry or distortion to the overall shape can be seen, suggesting possible minor gravitational interactions.
