The galaxy presents a largely smooth, elliptical morphology with minimal discernible substructure. A concentrated central bulge is observed, exhibiting a yellowish-orange hue, indicative of an older stellar population. The outer regions display a gradual decrease in luminosity, appearing more diffuse with subtle color variations suggesting the presence of some younger stars. The overall roundness suggests a classification leaning towards an E0-E3 type elliptical. There is no clear evidence of spiral arms, a prominent disk, or significant tidal disturbances. The galaxy appears relatively isolated with no obvious signs of interaction with neighboring galaxies, suggesting a quiescent evolutionary state.
