The galaxy appears to be a spiral galaxy viewed at a moderate inclination. A central bulge is clearly visible, exhibiting a bright, yellowish color, which suggests an older stellar population. Fainter spiral arms extend outwards from the central bulge. These arms appear to be somewhat diffuse, lacking sharp definition. There is evidence of bluer regions within these arms. The blue color implies the presence of ongoing star formation in these areas. The galaxy is relatively large, and the spiral structure has a smooth, grand design appearance. There are no obvious signs of major mergers or significant tidal disturbances.
