The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. It exhibits a yellowish-white hue, suggesting an older stellar population with lower levels of active star formation. The galaxy is generally round in appearance, with no distinct spiral arm structures or significant morphological disturbances visible. A very subtle extension of light appears on the right side of the galaxy, which could indicate a minor tidal feature or interaction. The overall form points towards a system that has largely completed its merging history and is in a relatively settled state.
