The galaxy presents a largely smooth morphology, potentially an elliptical or lenticular type. The central region exhibits a bright, concentrated core. The surrounding area displays a gradual decrease in luminosity, fading into the background. While there is some indication of faint disk-like structure, there appears to be no substantial spiral arm formation. The color profile suggests a population of older stars, potentially with limited ongoing star formation. Peripheral irregularities indicate the possibility of minor tidal distortions or previous merger events. 
