The galaxy presents as a spiral, with a relatively small, moderate central bulge. The spiral arms are tightly wound and defined by a mottled texture, suggesting active star formation regions. The overall ellipticity of the galaxy suggests an inclination relative to our line of sight. The bar is not prominent. The galaxy exhibits a disk-like structure. The system does not appear to be undergoing a major merger, although minor disturbances may be present. A bluer hue in the outer regions may indicate a population of younger, hotter stars within the spiral arms. The galaxy exhibits a central region of yellow and white, potentially indicating older stars.
