The galaxy presents as an elongated, disk-like structure with a fairly smooth overall appearance. The core exhibits a yellowish-orange hue, suggesting an older stellar population potentially dominated by red giant stars, and indicative of relatively low star formation activity. Extending outward from the core, a faint, diffuse disk is observed. There is a subtle color gradient from the core to the outer regions, with the outer disk appearing slightly bluer, perhaps indicating the presence of younger, hotter stars, though in small quantities. The morphology seems to be largely undisturbed. There are no prominent tidal features, strong spiral arms or obvious signs of a recent major merger event. The overall shape is neither perfectly round nor highly elongated, suggesting an intermediate ellipticity. The galaxy does not exhibit any indications of active galactic nuclei activity such as strong jets or a bright point source at the center.
