The galaxy exhibits a distinct spiral structure. Well-defined spiral arms are visible, with two primary arms appearing to originate from a central region. The winding of the spiral arms appears to be moderately open. The central bulge of the galaxy appears to be of moderate size and has an elongated, bar-like structure that extends through the central region. A significant portion of the galaxy's overall luminosity is concentrated in the central bulge and the inner portions of the spiral arms. Signs of galactic interaction can be observed, which appears to involve a smaller interacting galaxy. This smaller interacting galaxy may be disrupting the structure of the larger spiral galaxy.
