The galaxy presents a somewhat flattened, disk-like appearance, viewed at a slight angle relative to its plane. A central bulge region exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge is a fainter, bluish disk, which could be indicative of ongoing star formation or younger stars. The disk shows some irregularities or faint spiral arm structures, but the overall organization appears somewhat disrupted. There is a slight asymmetry to the outer regions of the disk, potentially suggesting gravitational interaction or a past minor merger event.
