The galaxy presents as a somewhat flocculent spiral with a relatively bright, concentrated central bulge. The bulge appears yellowish, suggestive of an older stellar population. The spiral arms are not well-defined, but are visible showing a bluish tint and some patchiness indicative of ongoing star formation. One side of the galaxy appears to have a slight tidal disturbance with a more distinct concentration of blue light, potentially caused by a minor interaction or recent accretion event. Overall, the galaxy is moderately inclined to our line of sight, and is of an intermediate size. 
