This galaxy presents a largely smooth morphology, suggesting an elliptical or lenticular classification. The light distribution is concentrated towards the center, exhibiting a bright, yellowish core. The galaxy appears almost perfectly round in shape, with minimal deviation from circular symmetry. There is little evidence of spiral arms, bars, or other distinct features typically associated with spiral galaxies. A faint, bluish halo surrounds the central core, possibly indicating the presence of a population of younger, bluer stars in the outer regions, or perhaps a more active star formation rate than expected in a typical elliptical galaxy. There is no obvious sign of ongoing merging or tidal disturbances. 
