The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated light profile with a bright, well-defined central bulge. The galaxy appears elongated, with a minor axis approximately one-third the length of the major axis. The color gradient transitions from a yellowish-white core to a bluer halo. No distinct spiral arms, dust lanes, or active star-forming regions are discernible, suggesting a population of older stars and relatively low star formation rate. The overall structure indicates a gravitationally settled system, possibly an evolved galaxy. Evidence of minor tidal disturbances cannot be ruled out. The morphology is consistent with a galaxy that has undergone significant merging and/or quenching of star formation.
