The galaxy presents a somewhat diffuse morphology, exhibiting characteristics of a spiral galaxy, though its arms are not sharply defined. The disk appears to be viewed at a moderate angle, allowing for a partial view of its structure. The galaxy's color profile indicates a mix of stellar populations. Blue hues are present, suggesting the presence of younger, hotter stars, particularly in regions that may correspond to spiral arms. However, the galaxy also exhibits more yellow and red regions, which may indicate older stellar populations or dust obscuration. The central bulge appears relatively small compared to the overall disk size. There is evidence of recent or ongoing star formation, particularly along the disk, as indicated by the presence of slightly brighter knots which could be HII regions. No strong bar feature is evident. It's possible there is a slight interaction or disturbance happening with the shape of the spiral arms, but no strong evidence of a merger or major disturbance is visible.
