The galaxy appears to be a spiral galaxy, characterized by a central bulge and a flattened disk. The bulge exhibits a concentrated brightness, suggesting a significant population of older stars. Emanating from the bulge are spiral arms that are relatively well-defined, though somewhat flocculent in nature. These arms display a bluer color, indicating ongoing star formation and the presence of younger, hotter stars. There is a slight asymmetry in the arm structure, possibly hinting at past interactions or internal dynamical processes. Dust lanes are subtly visible within the disk, obscuring some of the starlight and further highlighting the spiral structure. The overall color index suggests a mix of stellar populations, with both actively star-forming regions and older, more evolved areas. The galaxy's ellipticity is noticeable, but it is viewed at a relatively high inclination angle.
