The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a concentrated brightness, gradually fading into the outer regions. The galaxy's color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. There is little indication of spiral arms or significant dust lanes. The galaxy is relatively compact, with a somewhat rounded shape. There are no visually apparent signs of a major ongoing merger or significant tidal disturbances, although there is the possibility of a minor interaction based on the shape. Overall, the galaxy appears to be a well-formed elliptical galaxy with a substantial mass, a relatively low star formation rate, and a predominantly old stellar population.
