The galaxy presents as a spiral type, with a predominantly blue hue indicative of ongoing star formation. Two distinct spiral arms are observed emanating from a somewhat ill-defined, but present, central bulge. The arms exhibit a moderate degree of winding. The presence of a bar structure appears evident, extending across the center of the galaxy. The galaxy's disk is viewed at an angle. Evident irregularities in the disk suggest possible minor gravitational interactions or disturbances. The bulge appears to be of moderate size relative to the overall galactic disk. Overall color suggests a relatively young stellar population.
