The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light distribution. There are no discernible spiral arms or prominent dust lanes. The color profile suggests an older stellar population, with a yellowish-gold hue dominating the central region. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. There is a small, faint concentration of blue light in the bottom section of the galaxy, indicating potential younger star formations or small-scale galactic interaction. Overall, it appears to be a well-formed elliptical galaxy, relatively isolated and potentially in a quiescent state.
