The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density. There is a gradual decrease in luminosity towards the outer regions of the galaxy. The color profile indicates a yellowish core with hints of red, potentially indicating an older stellar population and/or dust obscuration. The outer regions appear bluer, which may suggest the presence of younger stars and active star formation in these areas, although the overall star formation rate appears to be low. There are no apparent signs of a major ongoing merger, or a strong tidal disturbance. The galaxy exhibits a morphology that trends toward round rather than highly elongated or disk-like. Based on the image, this galaxy appears to be a relatively massive system.
