The galaxy presents as a relatively compact object with a flattened, elongated morphology. A prominent central bulge or core is observed, exhibiting a yellowish-white hue, suggesting a population of older stars. Extending from this core are fainter, diffuse structures which might be indicative of a galactic disk. These outer regions appear bluer than the core. There is also a hint of asymmetry or tidal disturbances. Overall, the galaxy appears to be at an intermediate redshift.
