The galaxy presents as a slightly oblong, diffuse structure. It exhibits a color gradient, transitioning from a yellowish-orange core region to fainter, bluer edges. There is a suggestion of asymmetry, with a possible extension or tidal feature visible on one side, which may indicate a past or ongoing interaction. The galaxy appears relatively isolated in the image, although a smaller, more compact object is visible in close proximity. The galaxy exhibits characteristics of disk galaxies but may be in an intermediate stage, with a star forming rate that could be considered normal relative to its mass. Some signs of recent disturbances or merger events cannot be ruled out.
