The galaxy presents as a diffuse, elongated structure. There is an asymmetrical distribution of light, with the majority concentrated in a broad band that spans nearly the entire image. This band shows significant variation in intensity, with several brighter areas embedded within the overall structure. These brighter areas appear to be somewhat clumpy, suggestive of regions of active star formation or dense stellar populations.

The galaxy displays a gradient in color, with a shift towards redder hues in a small region, possibly indicating an older stellar population or increased dust obscuration. The predominant green color suggests ongoing star formation. The overall shape is suggestive of a distorted or interacting system. There is a faint tail-like extension emanating, further indicating a possible interaction or tidal disturbance. The main body appears relatively smooth on a large scale, but closer inspection reveals irregularities and substructure. A very small amount of blue scattered throughout hints to some presence of hot, young stars.
