The galaxy presents as a disk galaxy, exhibiting a notable tilt relative to our line of sight. The central bulge appears prominent, with a concentrated brightness, suggesting a significant stellar population. The disk component is also notable, displaying a somewhat mottled texture and exhibiting indications of spiral arm structures, though these are not sharply defined. The color gradient across the galaxy suggests varying stellar populations, with the central bulge appearing yellower, potentially indicating older stars, and the outer disk displaying bluer tones, hinting at younger, hotter stars and ongoing star formation. The galaxy's overall structure seems relatively undisturbed, lacking obvious signs of major mergers or tidal interactions. However, a slight asymmetry in the disk could indicate minor gravitational disturbances or past interactions. 
