The galaxy presents a disk-like structure with a prominent, moderately sized central bulge. The disk component is viewed at an oblique angle, but not quite edge-on, allowing a discernible assessment of its spiral structure. Two major spiral arms are clearly visible, loosely wound and extending outwards from the central bulge. The colouration suggests a mix of stellar populations. The central bulge appears yellower, possibly indicating older stellar populations, while the spiral arms exhibit bluer hues, suggestive of ongoing star formation and younger, hotter stars. There are some indications of possible disturbances or minor interactions, but the overall structure is relatively well-defined. A bar structure is faintly visible bisecting the bulge.
