The galaxy presents as a spiral type, displaying a prominent central bulge that appears relatively bright and yellowish, indicative of an older stellar population. The disk component exhibits spiral arm structures, though they are somewhat flocculent and not sharply defined. Two main arms can be discerned, winding loosely around the bulge. There is a moderate inclination to our line of sight, with the galaxy appearing somewhat elongated. The galaxy is generally blue in colour, indicative of more active star formation. There is some asymmetry in the outer disk region, suggesting possible interactions or minor disturbances. Overall, the galaxy appears to be a fairly typical spiral galaxy with a relatively normal morphology.
