The galaxy presents as a disk-shaped structure, viewed at an oblique angle, showing a moderate inclination. The central bulge appears relatively prominent and exhibits a yellowish-white color, suggesting an older stellar population. The surrounding disk displays a bluer hue indicative of ongoing star formation. There is a slight asymmetry to the disk, indicating that it may be moderately disturbed. No clear spiral arm structure is immediately apparent, although some clumpy regions of enhanced brightness within the disk may represent nascent spiral features. The overall light distribution appears relatively smooth.
