This galaxy appears to be a spiral galaxy exhibiting a prominent, bright central bulge. The bulge has a concentrated luminous core. Spiral arms emanate from the central bulge, tightly wound around it, extending outwards into a relatively well-defined disk. The spiral arms display a clumpy structure, hinting at regions of active star formation, especially towards the inner parts of the arms, closest to the core. There is evidence of a bar-like structure. The disk appears relatively smooth and well-defined, with moderate dust lanes and areas of lower surface brightness interspersed between the spiral arms. Overall, the galaxy appears relatively face-on. The morphology suggests it is a relatively massive system. There is also some possibility of minor disturbance or merging.