The galaxy appears to be a spiral galaxy, with a discernible disk structure. The galaxy is oriented at an angle relative to our line of sight, but not perfectly edge on. The presence of spiral arms is suspected, with a relatively tight winding pattern. The arms appear somewhat flocculent in nature.

A central bulge is apparent, although not overly dominant. The bulge appears to be moderate in size relative to the overall disk, but there is likely an appreciable disk component as well. The galaxy does not exhibit obvious signs of a strong bar structure but a subtle asymmetry may be present, potentially indicative of a weak bar. There do not appear to be any signs of major ongoing mergers or significant disturbances in the overall morphology.

The color distribution across the galaxy suggests varying stellar populations, with bluer regions likely associated with younger stars in the spiral arms, and yellower tones in the bulge consistent with an older stellar population.
