The galaxy presents as a relatively faint, disk-shaped structure viewed nearly edge-on. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. The disk component is visible as a faint, extended structure surrounding the bulge. The disk appears relatively smooth, though subtle variations in light intensity are visible within it. Based on its apparent morphology, it may be a spiral galaxy, with the disk being too angled to identify spiral arms. Alternatively, it could be a lenticular galaxy. The edge-on view makes it difficult to ascertain any ongoing or recent merger activity with confidence, but the galaxy's morphology appears relatively undisturbed. The galaxy has an estimated effective radius of a few kiloparsecs. There is very little evidence of blue light, which is usually indicative of new star formation.
