The galaxy appears to be a relatively smooth, elliptical object. It presents a concentrated, roughly spherical shape, suggesting an early-type classification. The color profile indicates a population dominated by older stars, with a redder hue throughout the galaxy's visible extent. There is no discernible spiral arm structure or significant dust lane obscuration. A slight elongation can be perceived, although the overall shape remains predominantly round. No signs of active galactic nuclei activity are visible, nor is there any evidence of tidal disturbances or ongoing mergers. The galaxy appears to be an isolated system in a relatively quiescent state.
