The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge that appears approximately round. The color profile suggests a population of older stars, indicated by the reddish hue in the outskirts of the galaxy. Fainter, bluer regions can be observed suggesting ongoing or recent star formation. No significant spiral arm structure or prominent dust lanes are discernible. The galaxy exhibits a faint halo, gradually fading into the background sky. There is some evidence of minor disturbance in the outer regions but it does not appear to be undergoing a major merger.
