The galaxy presents as a spiral with a relatively high degree of organization in its arm structure. Two prominent spiral arms are readily discernible, extending from the central region outwards. The arm winding appears to be predominantly medium to loose. The central bulge exhibits a moderate size relative to the overall disk. A bar structure appears to be present within the central region, potentially influencing the morphology of the spiral arms. There does not appear to be a strong degree of asymmetry or significant tidal disturbances, however a minor disturbance is possible. The disk is viewed approximately face-on and contains many active star forming regions. The color suggests a bluer stellar population. 
