The galaxy presents as a lenticular, or possibly a spiral galaxy viewed edge-on. A bright, prominent central bulge dominates the visual appearance, exhibiting a yellowish-white hue indicative of an older stellar population. Extending outward from the bulge is a flattened disk, characterized by a bluer color gradient. This color difference suggests active or recent star formation within the disk. There is a subtle, though visible dust lane or feature running the length of the major axis of the disk. There is minimal evidence of strong spiral arm structures, the galaxy does display subtle disturbances in its structure, possibly resulting from a minor merger event in the past. The overall morphology suggests a transition type, possibly between a spiral and elliptical galaxy.
