The galaxy presents as a disk-shaped system, viewed at a moderate inclination, but closer to edge on. There is a prominent central bulge exhibiting a yellowish hue, suggesting an older stellar population. The disk component displays a bluer color, especially towards the outer edges, indicating the presence of younger, hotter stars and ongoing star formation. The disk structure appears relatively smooth, with hints of subtle spiral arm structure, but no prominent features. The galaxy appears to be generally undisturbed, showing no obvious signs of a major merger.
