The galaxy appears to be a relatively small, early-type system, potentially an elliptical or lenticular galaxy, viewed nearly edge-on. It exhibits a smooth, centrally concentrated light profile with a brighter core. There is a suggestion of a flattened shape, implying possible rotational support or a disky component, though clear spiral arm structures are absent. The galaxy's color is somewhat redder/yellower, indicating an older stellar population and a lack of significant recent star formation, correlating with its smooth appearance. Minor distortions in the outer regions are visible, suggesting a possible past interaction or minor merger event. The overall structure doesn’t appear to be undergoing any major merging activity.
