The galaxy presents as a flattened, disk-like structure with a significant central bulge. The disk appears relatively smooth, lacking prominent, well-defined spiral arms. There's a hint of bluer coloration tracing the outer edges of the disk, suggesting the presence of younger stellar populations possibly undergoing active star formation. The central bulge is notably redder in color, indicative of an older, more evolved stellar population. The overall morphology suggests an evolved galaxy with a substantial spheroidal component. There is no clear evidence of any major merger events or tidal disturbances. The galaxy's observed shape is close to round.
