The galaxy presents a generally smooth, rounded morphology. It appears to be an elliptical galaxy with no obvious spiral arm structures or distinct features such as dust lanes. A dominant central bulge is visible, exhibiting a bright, concentrated core.

The galaxy has a yellowish-white hue, indicative of an older stellar population with a relatively low star formation rate. The light is evenly distributed, suggesting a uniform population of stars.

There is a slight red color gradient observable outwards from the core, which could suggest a difference in the age or composition of the stars in the outer regions, or potentially some dust obscuration.

Overall, the galaxy appears to be a relatively undisturbed, evolved system.
