This galaxy appears to be a spiral galaxy, viewed at an oblique angle, not quite face-on or edge-on. A discernible disk structure is present. The central bulge exhibits a moderate size relative to the overall disk. The presence of spiral arms can be inferred, though they are not sharply defined, suggesting a flocculent or grand design spiral structure. Evidence of a bar feature is observed within the central region, appearing moderately prominent. The overall color distribution indicates an older stellar population in the bulge region, exhibiting a yellow to orange hue, which is indicative of evolved stars. Bluer regions are seen in the disk, particularly along the spiral arm structures, suggesting active star formation is occurring. The galaxy exhibits no apparent major tidal disturbances or interactions, although minor irregularities or asymmetries in the outer disk cannot be entirely ruled out. The galaxy displays a relatively smooth overall structure.
