The galaxy presents as a structured system exhibiting both smooth and featured components. The central region displays a concentrated, relatively smooth distribution of light, suggesting a prominent bulge or core. Extending from this central area, there appears to be evidence of a disk-like structure, though it's not sharply defined. Patches or arms of material are discernible, indicating ongoing star formation. The morphology is somewhere between round and elliptical, but closer to elliptical. There may be some signs of minor disturbances or tidal features that suggest possible interactions or past mergers with another galaxy. There is no evidence of a current major merger taking place.
