The galaxy appears to be a disk galaxy, viewed at an oblique angle. The central bulge is moderately sized and exhibits a yellow-white hue, suggesting an older stellar population. Surrounding the bulge is a fainter, broader disk. Faint spiral arm structures may be present, but are not well-defined. The disk component shows a mottled texture with a mix of blue and greenish regions. This suggests a blend of both older stars and some ongoing star formation. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, although minor asymmetries cannot be ruled out. Overall, the galaxy appears relatively undisturbed, with a bulge-dominated disk and hints of recent, but not vigorous, star formation. 
