The galaxy presents as a grand design spiral galaxy with a notably bright and moderately sized central bulge. The spiral arms are well-defined, demonstrating a two-armed structure that winds relatively tightly around the galactic core. Patches of bluer light suggest regions of active star formation within the arms. The presence of a bar is evident, bisecting the bulge. There is no major visual disturbance in the disk, but perhaps minor tidal interactions given the slight asymmetry of the arms. The overall color profile is dominated by light towards the redder end of the spectrum, particularly within the bulge and inner regions of the spiral arms, indicating an older stellar population.
