The galaxy presents as a spiral structure with prominent, well-defined arms emanating from a central bulge. These arms exhibit a tightly wound morphology. A distinct bar feature appears to bisect the bulge, running along its major axis. The central bulge is relatively small compared to the overall galactic disk and appears to be more luminous. Star formation appears active within the spiral arms, evidenced by the presence of numerous bright regions. The galaxy does not show obvious signs of a major ongoing merger. There are some small disturbances, but there is no clear, large-scale tidal deformation.
