This galaxy appears to be a relatively smooth, disk-like galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A slightly inclined disk extends from the central bulge, and the disk exhibits a bluer color compared to the bulge, which indicates the presence of younger stars and ongoing star formation. The galaxy does not show any strong spiral arm structures but appears slightly disturbed on one side, suggesting a minor interaction or internal process. Overall, the galaxy presents as a moderately luminous system at a considerable distance, exhibiting a mix of evolved and young stellar populations.
