The galaxy appears as a centrally concentrated elliptical type with a smooth overall morphology. It has a fairly homogenous distribution of light, with a gradual decrease in intensity from the core outwards. There is a slight ellipticity observed with the major axis oriented approximately northwest to southeast. The color profile suggests an older stellar population. The galaxy exhibits a redder hue in the central region, transitioning to slightly bluer colors further out. The galaxy shows no obvious signs of active star formation, such as bright HII regions or spiral arm structures. There is no apparent interaction with other galaxies or significant morphological distortions.
