The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge, tracing an approximately symmetric pattern. The arms exhibit a somewhat flocculent structure, showing areas of enhanced luminosity, likely regions of active star formation. The color gradients within the arms suggest varying stellar populations, with bluer hues indicating younger stars. The central bulge is luminous and slightly elongated. There is evidence of a bar-like structure spanning the central region. The disk is viewed at a slight inclination. No significant signs of tidal interactions or major disturbances are evident in the immediate vicinity of the galaxy.
