The galaxy appears to be a spiral galaxy, viewed edge-on. A prominent central bulge is visible, exhibiting a yellowish hue that likely indicates an older stellar population. The disk is thin and elongated, displaying a bluer tint along its outer edges, potentially signifying ongoing star formation. There is a noticeable dust lane bisecting the galaxy, obscuring the light from the bulge. Overall, the galaxy shows no signs of significant tidal disturbances or major merger activity, with a relatively smooth and undisturbed morphology.
