The galaxy appears as a single, relatively smooth object. Its morphology suggests a spheroid-like structure with minimal discernible features such as spiral arms or a distinct bar. The galaxy's light distribution is concentrated towards the center, exhibiting a bright, compact core. A slight elongation is visible, indicating it is not perfectly spherical, appearing somewhat elliptical in shape. A subtle color gradient exists, with a yellowish-white central region transitioning to a bluer hue in the outer regions. This color difference might imply variations in stellar populations, potentially with older, redder stars concentrated in the core and younger, bluer stars in the surrounding regions. There is no obvious evidence of any significant ongoing merger activity or major disturbances in the galaxy's structure.
