The galaxy presents as a relatively smooth, elongated structure. Its color profile suggests a prominent central bulge with a yellowish-orange hue, indicating a population of older, cooler stars. Fainter, bluer regions are observed extending outwards from the central bulge, hinting at areas of ongoing star formation within a possible disk-like structure. The disk appears to be viewed at a high inclination, close to edge-on. There are slight disturbances in the edges of the disk, but on the whole, the galaxy looks to be quite settled and without major mergers or disturbances.
