The galaxy presents as a disk-shaped structure, with a moderate inclination relative to our line of sight. A prominent central bulge is observed, exhibiting a smooth, concentrated light profile that suggests an older stellar population. The disk component shows some hints of spiral structure, though it appears somewhat flocculent, lacking well-defined, grand-design arms.

The color gradient across the galaxy indicates variations in stellar populations and dust content. The bulge exhibits a yellower hue, likely due to older, redder stars, while the disk is bluer, suggesting the presence of younger, hotter stars and ongoing star formation. There are disturbances within the galaxy, but they appear to be minor.
