The galaxy presents as a relatively bright, elongated structure, with an apparent edge-on orientation relative to our line of sight. There is a distinct central bulge, appearing bright and somewhat yellow. A fainter disk component extends from the central bulge. The disk is not perfectly uniform, showing hints of dust lanes or patchy star formation. The disk itself seems relatively thin and well-defined, though moderately obscured by dust. The overall morphology suggests a spiral galaxy, likely of late-type with a tightly wound disk. No prominent tidal features or signs of recent major mergers are apparent.
