The galaxy presents as a relatively small spiral with a moderate inclination. The central bulge appears significant, contributing substantially to the overall luminosity of the galaxy. Faint spiral arms can be discerned, extending from the central region. These arms display a somewhat patchy appearance, suggesting active star formation regions. The color profile indicates a bluer hue, especially pronounced within the arms, pointing towards a population of younger, hotter stars. The galaxy's overall structure indicates a rotating disk with a flattened morphology. A bar structure seems present, bisecting the central bulge. The galaxy's outskirts display a diffuse halo, gradually fading into the background sky. No obvious signs of recent major merger activity are apparent, but minor disturbances may exist.
