The galaxy presents an overall elliptical morphology, exhibiting a smooth and relatively featureless structure. The light distribution appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. The galaxy's color profile shows a predominantly redder hue in the central regions, potentially indicating an older stellar population. Fainter bluish tinges can be observed in the outermost regions, hinting at the presence of younger, hotter stars, but not to a significant degree. There is no apparent spiral arm structure, nor any signs of a prominent galactic disk. There is no visually significant sign of any ongoing merger activity or strong tidal disturbances and the general shape is fairly regular, not strongly elongated or cigar shaped. The overall roundness of the light distribution appears neither perfectly circular nor highly flattened.
