This galaxy presents as a spiral type, exhibiting a defined disk structure. Two spiral arms are clearly visible, extending from a central bulge region. The winding of the spiral arms appears to be moderately loose. The central bulge appears to be of moderate size, but not dominant. A bar structure appears to be present, showing to be weak/moderate. Overall, the morphology suggests a galaxy that is not undergoing any major merging events, though some minor disturbances cannot be ruled out based on the irregularity of the disk shape. Star formation appears to be active, evidenced by the color, particularly in the spiral arms, compared to the bulge. The galaxy is seen nearly face on.
