This galaxy presents a somewhat irregular, disk-like morphology with a relatively bright central region. A distinct feature is a surrounding ring-like structure that appears less uniform in color and intensity. The distribution of light within the galaxy seems relatively uneven, lacking a clearly defined spiral arm structure, and a noticeable degree of disturbance is indicated by the galaxy's irregular shape, which is somewhat elongated and not perfectly symmetrical. The central bulge appears prominent, possibly indicating a significant population of older stars. There's a subtle color gradient, hinting at varying stellar populations or dust distribution across the galaxy. Given the disturbances and irregular morphology, there could be ongoing or past interaction with another galaxy.
