The galaxy presents a somewhat elliptical morphology. A central bulge region is visible, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Surrounding the bulge is a disk-like structure, characterized by a bluer color, indicating the presence of younger, hotter stars and potentially ongoing star formation. The spiral arms are not well-defined, appearing rather patchy and flocculent, with a low surface brightness. There are some hints of disturbances in the disk. Overall, the galaxy's structure suggests it is neither a perfectly smooth elliptical nor a grand design spiral, but something in between, possibly a galaxy that has experienced some minor interactions.
