The galaxy presents a flattened, disk-like morphology, viewed at a nearly edge-on orientation. While the image resolution limits detailed structural analysis, there is tentative evidence of spiral arm features. A central bulge is faintly visible, exhibiting a moderate concentration of light. The disk shows a gradual fading in intensity from the core outward. The overall color appears to be skewed slightly toward the redder end of the spectrum. There is some indication of ongoing star formation activity, though without higher resolution imaging or spectroscopic data, the spatial distribution and intensity remain uncertain. The galaxy shows evidence of a recent or ongoing merger.
