The galaxy exhibits a predominantly smooth morphology. The central region displays a high concentration of light, appearing as a bright, yellowish core. Moving outwards from the core, the intensity of light gradually diminishes, transitioning into a more diffuse halo. Hints of bluer light are observed in the outer regions of the galaxy, potentially indicating regions of recent star formation. The overall shape is somewhat elliptical, leaning more towards a flattened spheroid rather than a distinct disk structure. There's a slight asymmetry in the outer halo, but the galaxy does not appear to be undergoing any major merger events, though some minor disturbances cannot be ruled out. No prominent spiral arms or bar structures are discernible.
