The galaxy presents a clear spiral morphology, with a prominent disk structure oriented at a moderate inclination relative to our line of sight. The central bulge appears moderate in size and exhibits a yellowish hue, suggesting an older stellar population. Two distinct, tightly wound spiral arms are visible, emanating from the central region and extending outwards into the galactic disk. These arms exhibit a bluer color, indicative of ongoing star formation. There is no obvious presence of a central bar structure. No signs of major mergers or significant tidal disturbances are apparent, although some minor irregularities are present, which could potentially point to a weak interaction. The disk appears relatively smooth, although the presence of spiral structure suggests it is not entirely uniform. The overall appearance suggests a relatively normal spiral galaxy undergoing active, but not extreme, star formation. The galaxy displays an estimated diameter of approximately 6.6 kpc.
