The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical. The light profile exhibits a gradual decline in intensity from the core outwards, indicative of a well-established stellar population. The overall color is slightly redder. There is no discernible spiral structure, bar, or significant dust lane present. The galaxy appears to be fairly isolated and does not show strong signs of tidal interaction or recent merger events. It has a relatively low star formation rate.
