The galaxy presents as a spiral type, characterized by a discernible disk and a moderately sized bulge. The spiral arms appear distinct and well-defined, exhibiting a tightly wound morphology. There is a presence of a bar-like structure spanning a noticeable portion of the galaxy's central region. Evident is a slight degree of asymmetry or disturbance to the galactic structure, suggestive of a possible minor interaction with another galactic body or a recent merger event. The color distribution across the galaxy indicates a relatively older stellar population, with the majority of stars residing in the central bulge. Additionally, there are two red spots below the galaxy, which show active star forming regions.
