The galaxy presents as a relatively smooth, elliptical object. It appears to be spheroidal in shape, displaying high central concentration. The color profile suggests a higher proportion of older stars, with a yellowish-red hue dominating. There is minimal indication of spiral arm structures or significant dust lanes. The galaxy exhibits a degree of roundness, with a near lack of elongation, indicating that it is likely an E0-E3 galaxy. There are no obvious signs of tidal disturbances or ongoing major merger events.
