The galaxy presents a distinct spiral structure, characterized by well-defined arms extending from a central bulge. The spiral arms exhibit a moderate to tight winding pattern. The color distribution suggests active star formation within the arms, indicated by a bluer hue, particularly in the outer regions. A central, bright bulge is visible. No significant bar structure is discernible. The overall morphology suggests a classification of a spiral galaxy, with some indication of ongoing star formation activity. The galaxy appears relatively undisturbed.
