The galaxy exhibits a prominent disk structure, viewed at an oblique angle. Spiral arms are visible, although not sharply defined, winding outwards from a central bulge. The bulge appears moderately sized relative to the overall disk. A bar-like structure seems to be present within the central region, exhibiting moderate strength. The overall color profile suggests ongoing star formation, with a significant contribution from older stellar populations, giving the galaxy a yellow/white hue in the central regions fading to blue in the outer disk. No signs of major mergers or strong tidal disturbances are apparent; however, the morphology suggests potential minor disturbances. The disk appears mostly continuous, with only slight asymmetries, likely indicating weak interactions. The galaxy's shape is overall well-defined, suggesting a relatively undisturbed morphology.
