This galaxy presents as a spiral type, although the arms are somewhat tightly wound and not sharply defined. The central bulge appears to be of moderate size, showing a notable concentration of light. There is evidence of a bar structure crossing through the central region. The disk of the galaxy exhibits some disturbances or irregularities. Color gradients suggest active star formation regions interspersed within the spiral arms. Overall, the galaxy does not appear to be undergoing a major merging event, but there might be evidence of minor gravitational interactions or disturbances.
