The galaxy appears to be a spiral galaxy, viewed at an oblique angle. A central bulge is apparent, exhibiting a yellowish hue, possibly indicative of an older stellar population. Surrounding the bulge is a disk, though its detailed structure is somewhat indistinct due to the viewing angle and resolution. Faint spiral arm structures can be inferred, with a suggestion of moderate winding. The blue tint in the disk implies ongoing star formation. There is no obvious visual evidence of a strong bar structure. The overall morphology suggests a relatively undisturbed system, with no prominent signs of recent major merger activity.
