The galaxy appears to be a disk galaxy, viewed at a somewhat oblique angle. There is a central bulge with a yellowish hue, indicating an older stellar population. The disk shows evidence of spiral arm structure, but these features are somewhat diffuse and not sharply defined. The disk exhibits bluer colors, particularly on one side, suggesting the presence of younger, hotter stars and ongoing star formation. Some irregular features or disturbances are apparent, possibly indicative of minor interactions or internal processes affecting the galactic structure. The overall shape of the galaxy is elongated, but not extremely so, with a moderate aspect ratio. There is one noticeable condensation to the south of the center, possibly a region of enhanced star formation or a smaller companion galaxy. The color gradients from the center to the outer regions support a radially decreasing stellar age profile.
