The galaxy presents as a spiral type, not viewed edge-on. A prominent central bulge is apparent, displaying a yellowish hue, suggestive of an older stellar population. Two distinct spiral arms emanate from the central region, displaying a well-defined structure and wrapping moderately around the bulge. The arms themselves exhibit a bluer color, indicative of ongoing star formation within them. A bar structure is observed through the center of the bulge. Overall there are no indications of any major merging events.
