The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, suggesting a significant bulge component. There is a subtle disklike component that can be inferred from its elongated shape and the increased blueness in the outer regions of the galaxy. The color gradient suggests that the central region hosts an older stellar population, while younger, bluer stars reside in the outer regions. Faint tidal features or minor disturbances seem present within the galaxy's halo, indicating past or ongoing gravitational interactions. The galaxy does not exhibit strong signs of active star formation. There are some reddish regions on one side of the galaxy, that may imply dust or more likely a region of older stars.
