This galaxy presents as a spiral galaxy with an inclination towards edge-on. The central bulge exhibits a high surface brightness with a golden hue. Faint spiral arms emerge from the central region, appearing somewhat tightly wound. These arms exhibit clumpy regions of star formation, indicated by a bluer color. The disk component appears significantly larger than the bulge, with an elongated morphology that supports the impression of a nearly edge-on orientation. Evidence of a bar structure is subtle, but may be present. There might be minor disturbances in the disk, possibly indicating interaction with a smaller object. The light distribution suggests an older stellar population dominates the central bulge, while younger, hotter stars are prominent within the spiral arms.
