The galaxy presents as a spiral type with a fairly bright, prominent bulge. Two distinct spiral arms appear to emanate from the central bulge, displaying a loosely wound morphology. The arms are somewhat diffuse and asymmetric, suggesting potential gravitational interactions or past merger events. The overall color profile of the galaxy indicates the presence of both older stellar populations in the bulge, exhibiting yellowish hues, and regions of ongoing star formation within the spiral arms, characterized by slightly bluer tones. The disk is viewed at a moderate inclination. Evidence suggests a possible weak bar structure in the galaxy's central region.
