The galaxy presents as a somewhat amorphous, diffuse structure with a concentrated central region. The light distribution suggests a general spheroidal shape, but with irregular edges that deviate from perfect ellipticity. A discernible core exists, exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter, bluer regions extending outwards from the central concentration hint at more recent star formation in the outer regions. The overall color gradient suggests a radial trend in stellar population age, with older stars concentrated in the center and younger stars in the periphery. Minor disturbances are visible within the galaxy's structure, such as slight irregularities in the outer regions of the disk. No prominent spiral arms are evident.
