The galaxy presents as a spiral galaxy with a moderately sized central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Prominent spiral arms extend outwards from the central region, exhibiting a bluer color, which indicates the presence of younger, hotter stars and ongoing star formation. The arms appear somewhat loosely wound and display some patchiness, possibly due to variations in star formation density or dust obscuration. The disk is viewed at a slight angle relative to edge-on. There's no sign of merging and the galaxy appears to be relatively undisturbed. A faint bar structure is potentially present within the central region. 
