The galaxy exhibits a spiral morphology. Two prominent spiral arms are visible, displaying a relatively tight winding pattern. The presence of a central bulge of moderate size can be observed, though it appears to be somewhat indistinct. There may be a weak bar-like structure traversing the central region, but further analysis is needed to confirm its presence and strength. The overall structure seems to be experiencing a minor disturbance, possibly hinting at an ongoing or recent interaction, but no major tidal features are clearly visible. The disk is oriented at a slight angle relative to our line of sight. There appears to be ongoing star formation occurring within the spiral arms.