The galaxy presents as a spiral type, exhibiting well-defined spiral arms. These arms are tightly wound, indicating a potentially high shear rate within the galactic disk. The arms are not perfectly symmetrical, suggesting possible interactions or internal asymmetries affecting the galaxy's morphology. The central bulge appears relatively small, with no apparent bar structure. The galaxy disk is presented face-on. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major merging activity. The spiral structure is generally smooth, with limited indication of significant star-forming regions along the arms. The galaxy possesses a blue hue, indicating ongoing star formation. The estimated physical size indicates this is a small galaxy.
