The galaxy presents as a generally smooth, elliptical morphology. There is a concentrated central bulge that appears yellowish-white in color. This central region transitions to a less concentrated halo extending outwards, exhibiting a slightly reddish hue. The galaxy displays a predominantly spheroidal shape, with minimal discernible features suggesting the presence of a distinct disk structure. There is no evidence of any major tidal disturbances or ongoing merger activity, although some minor irregularities in the outer halo cannot be ruled out with this image quality. The light distribution suggests a relatively evolved stellar population, with potentially ongoing, albeit modest, star formation.
