The galaxy presents as a somewhat amorphous, diffuse structure. The light distribution appears largely smooth, lacking prominent spiral arms or a well-defined central bulge. There is a slight elongation, but it's difficult to determine a precise morphological classification. The object displays a broad color gradient, ranging from bluer hues in what appears to be the core region, transitioning to redder tones in the outer regions. The distribution of light in the galaxy is moderately concentrated towards the center, which may be indicative of on-going or recent star formation. There is no obvious signs of dust lanes or other fine scale features within the galaxy. The outskirts of the object appear to fade out gradually, suggesting an extended halo or envelope of stars, possibly in a process of merging. The observed colors are consistent with a galaxy at a moderate redshift. Overall, the galaxy appears to be relatively undisturbed morphologically, but with some blue light indicating recent star formation.
