The galaxy presents a generally smooth, elliptical morphology. The core exhibits a high degree of spheroidal symmetry with a diffuse radial intensity gradient. The outer regions display a subtle elongation, with an intermediate, non-circular shape. No obvious spiral arm structures or prominent dust lanes are discernible. There are no apparent signs of ongoing major mergers or significant tidal disturbances. There are no noticeable irregularities in the overall shape and appearance of the galaxy. The galaxy appears to be relatively quiescent with potentially low current star formation. The color indices suggest a population dominated by older stars. The approximate estimated size is around 4 kpc. The galaxy displays a magnitude around 18 in the DESI r-band.
