This galaxy appears to be an edge-on spiral galaxy, exhibiting a prominent, elongated disk structure. There is a central bulge, which seems somewhat boxy in nature, although a rounded component is also apparent. The disk shows evidence of dust lanes, particularly noticeable as dark obscurations bisecting the galaxy's light. The overall color gradient suggests a redder central region, possibly indicating an older stellar population in the bulge, transitioning to bluer hues in the outer disk, indicative of ongoing star formation. The morphology is relatively undisturbed, with no immediately obvious signs of major mergers or strong tidal interactions. There may be slight distortions in the disk, suggesting possible minor interactions, but this requires further investigation.
