The galaxy appears to be a spiral galaxy, observed edge-on. There is evidence of a central bulge, though it is not prominently defined. The disk is elongated and exhibits a mottled texture, suggesting the presence of dust lanes. The color gradient transitions from a bluer hue at the apparent edges of the disk to a redder hue towards the center, which is indicative of differential stellar populations and dust obscuration. No distinct spiral arms are visible, potentially due to the edge-on view obscuring the disk's structure. There is a faint indication of ongoing star formation, as suggested by the blue light. No signs of any major ongoing merger events, or any significant distortions in the shape of the galaxy are present. Overall, the galaxy presents a relatively undisturbed and quiescent morphology.
