The galaxy presents a flattened, elliptical morphology. A bright, concentrated nucleus is visible, suggesting a central bulge component. The disk appears relatively smooth, with no readily apparent spiral arm structures. The color profile indicates a dominance of older stellar populations, as evidenced by the redder hues observed throughout the galaxy, particularly within the central bulge. There is a distinct lack of blue star formation regions. The galaxy's overall shape is elongated, with a high degree of axial ratio suggesting a nearly edge-on orientation relative to our line of sight. No significant signs of tidal disturbances or ongoing mergers are immediately observable. The galactic halo appears diffuse and extends modestly beyond the main disk.
