The galaxy presents as a reddish-orange elongated structure, suggesting it is being viewed edge-on. There is a noticeable central bulge that appears to be moderately prominent and somewhat rounded. The galaxy exhibits a disk-like morphology with a high degree of inclination relative to our line of sight. This disk shows a relatively smooth texture. Evident is some minor disturbance in the disk, but overall the disk appears stable with no clear signs of major merger activity. The color profile indicates a likely evolved stellar population. Blue light, likely from younger stars, is present in a region close to the disk. This hints at ongoing star formation within a galaxy that is otherwise undergoing quiescence.
