The galaxy presents as an edge-on spiral, characterized by a prominent central bulge exhibiting a yellowish-orange hue. The disk, viewed nearly edge-on, appears relatively thin and extended, displaying subtle variations in color suggesting the presence of dust lanes and varying stellar populations. The bulge appears smooth and largely symmetrical, indicating a well-established stellar population. There is no visually apparent evidence of strong tidal interactions or recent major mergers. Faint hints of a boxy bulge may be present, but this is uncertain based on the image resolution. The disk color suggests ongoing, albeit potentially limited, star formation activity. The overall impression is of a galaxy with a well-defined structure, undisturbed morphology and likely a moderate rate of star formation.
