The galaxy exhibits a roughly elliptical morphology with a bright, concentrated central region. It displays a disk-like structure viewed at an oblique angle; internal structure suggests the presence of spiral arms, although they are not well-defined. The central bulge exhibits a bright, luminous appearance. Faint, diffuse emission extends outwards from the main body of the galaxy, potentially indicating a halo structure. Overall, the galaxy appears relatively smooth, though some subtle irregularities could indicate possible interactions or tidal features. The color gradient suggests varying stellar populations, with bluer hues in some areas and redder hues in others. This may indicate ongoing star formation.
