The galaxy appears to be a spiral galaxy, potentially with a bar structure. The spiral arms are relatively tightly wound, with a considerable presence of blue star forming regions. The bulge has a relatively small size, but is noticeable, and the galaxy presents a high overall disk fraction. There is no indication of a major ongoing merger, although the disk exhibits some morphological disturbances suggesting a previous minor interaction. The central region is yellow, likely indicating an older stellar population and dust presence.
