The galaxy exhibits a largely smooth morphology with a relatively high degree of central concentration. The color profile suggests a range of stellar populations, with a redder core potentially indicating older, more evolved stars. A bluer halo surrounds the central region, possibly indicating the presence of younger, hotter stars and ongoing star formation. There is a slight asymmetry, but the overall shape is generally elliptical. There's no clear evidence of spiral arms or a prominent disk component; the galaxy appears more spheroidal in nature. There's no visual evidence of any major ongoing merger activity or significant tidal disturbances, and there is a lack of extended features suggesting interactions.
