The galaxy presents as a spiral galaxy with a redshift of approximately 0.11. It is inclined somewhat to our line of sight, allowing for a partial view of its spiral structure. The spiral arms appear tightly wound and extend outward from a central bulge. The bulge is a moderate size relative to the overall galaxy, appearing neither dominant nor particularly small.

Evidence of active star formation is present within the spiral arms, indicated by the observed color gradients. The galaxy does not exhibit strong evidence of a bar structure. The overall morphology suggests a galaxy undergoing normal spiral structure evolution, without significant signs of major mergers or disturbances. There is a suggestion of a faint outer halo surrounding the main galactic disk.
