The galaxy presents as a spiral galaxy with a notable bar structure traversing its central region. The bar appears moderately strong, and is seen as somewhat elongated. A bright, concentrated central bulge is observed within the inner region of the galaxy, indicating a relatively high density of stars at the core. Two spiral arms are clearly discernable as they extend outward from the bar and bulge. These arms appear distinct, with a medium degree of winding.

The color distribution suggests ongoing star formation, particularly within the spiral arms, indicated by bluer hues. The spiral arms have some knotty blue regions, which supports this. The central bulge exhibits a more yellowish/redder tint, possibly representing a population of older, redder stars. There is no obvious indication of major or disruptive merging, but some minor disturbances may be present in the outer spiral arms. 
