The galaxy presents as a spiral type, though moderately inclined relative to our line of sight. A central bulge is discernible, exhibiting a yellow-white hue, suggesting an older stellar population within the nucleus. Extending outwards from the bulge are spiral arms, which appear somewhat tightly wound and have a blue tint, indicating ongoing star formation.

The disk of the galaxy, while clearly present, seems relatively smooth, hinting at a moderate level of star formation activity. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances; it is relatively undisturbed in its morphology. A bar feature is possibly present. The galaxy displays a relatively high degree of ellipticity.
