The galaxy exhibits an overall elongated morphology, suggestive of a disk galaxy viewed at an oblique angle. The light distribution is not uniform. One end presents a brighter, more concentrated region, with a yellow-greenish tint, potentially indicative of a higher density of older stellar populations and possibly ongoing star formation. Moving towards the opposite end, the light becomes more diffuse and blue-tinged, which could be caused by younger, hotter stars. This distribution could also be evidence of a recent or ongoing merger event. A slight curvature or warping of the galaxy's disk is also possible.
