This galaxy presents as a spiral galaxy with a prominent central bulge. The bulge appears bright and somewhat spherical, suggesting a significant population of older stars. A disk component is clearly visible, oriented at an oblique angle to our line of sight. Spiral arms are present and appear tightly wound around the bulge, displaying a predominantly two-armed structure. Indications of star formation regions are visible within the spiral arms, appearing as localized areas of slightly enhanced blue light. The overall color of the disk is relatively uniform, indicating a well-mixed stellar population. There is no readily apparent evidence of a strong bar structure, nor is there any obvious indication of major merging activity or significant tidal disturbances. The spiral structure is well-defined, although somewhat compact in appearance, with no indications of grand design features. Overall, the galaxy appears to be a well-formed, relatively undisturbed spiral galaxy.
