The galaxy presents as a spiral type with a moderately sized bulge relative to the disk. Two distinct spiral arms emerge from the central bulge, displaying a medium winding. No obvious bar structure is observed in the central region. The color of the central bulge is yellowish, suggesting an older stellar population. The spiral arms exhibit a bluer hue, indicative of ongoing star formation. There is no evidence of any major merging events or significant disturbances in the overall structure. The galaxy appears to be fairly face-on with respect to our line of sight.