The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The core region exhibits a high degree of luminosity, possibly indicating the presence of an active galactic nucleus or a dense concentration of stars. Extending outward from the core, the galaxy displays a somewhat flattened or elliptical structure. There is a slight suggestion of disturbances in the galactic disk. Overall, the galaxy presents as a non-complex, relatively symmetrical system with a notable central bulge. Further investigation would be needed to determine its exact morphological classification and evolutionary state.
