The galaxy presents a generally smooth, elliptical morphology. The central region displays a high concentration of luminosity, appearing bright and relatively spherical. A fainter, more diffuse halo extends outwards.  There is some indication of asymmetry, potentially due to minor tidal disturbances or an ongoing minor merger. One area of higher concentration of redder light can be observed along the outer edges of the disk. This could possibly be older stars or dust in that region. The galaxy exhibits colors across the g, r, and z bands, with a slightly redder appearance overall. This would suggest a moderately evolved stellar population and a low rate of on-going star formation.