The galaxy presents as a spiral type, with a significant disk component exhibiting clearly defined spiral arms. These arms appear to be tightly wound towards the central region, possibly indicating a relatively old stellar population within the spiral structures. The central bulge is discernible but does not dominate the overall structure, suggesting it is a relatively small bulge.

The galaxy is viewed at a shallow angle, not quite edge-on. The color distribution across the galaxy shows a concentration of yellower light toward the center, likely corresponding to older stars in the bulge. The spiral arms display regions of bluer light indicative of younger star formation. Overall the galaxy does not exhibit any signs of recent major mergers or significant tidal disturbances.
