The galaxy presents as a spiral type, exhibiting a prominent disk structure. Two distinct spiral arms are observed, moderately wound around the central bulge. A bar-like structure is suspected bisecting the bulge, with moderate prominence. The bulge appears to be a moderate size, contributing significantly to the overall luminosity of the galaxy. Traces of possible recent minor disturbances are present. The majority of the light seems to be emanating from the center, and the galaxy is most likely not undergoing any major mergers or major disturbances.