The galaxy presents as a slightly inclined disk galaxy. Prominent spiral arm structures are visible, though somewhat diffuse, indicating ongoing star formation. The disk exhibits a bluer color, consistent with a population of younger stars. A central bulge component is present, appearing relatively small in proportion to the disk, with a somewhat indistinct structure, fading into the spiral arms. There is a possibility of a central bar structure, though this is subtle. There appears to be minor disturbance in the outer edges of the disk. Overall, the galaxy exhibits a relatively smooth appearance suggesting that this is an old galaxy with relatively low star formation, with no signs of major ongoing merger events.
