The galaxy presents as a spiral structure with a prominent central bulge. Two distinct spiral arms are visible, exhibiting a medium winding pattern. The arms appear somewhat diffuse, showing regions of active star formation. The bar structure is subtly noticeable, with a somewhat elongated central bulge. Overall the galaxy appears to be relatively isolated, showing no major signs of recent merger activity. There are some minor disturbances visible. The core appears to be bright and centralized, gradually fading outwards into the spiral arms.
