The galaxy presents a clear spiral structure, with a dominant, moderately-sized bulge. Two distinct spiral arms are observable, exhibiting a loose winding pattern. There are indications of potential disturbances in the galaxy's morphology, suggestive of a possible ongoing or recent interaction with another galaxy. The central bulge appears yellowish, possibly indicating an older stellar population, while bluer regions are visible within the spiral arms, likely corresponding to younger stars and star-forming regions. The galaxy is relatively faint and compact.