The galaxy appears as a roughly circular, relatively smooth object. Its light profile suggests a centrally concentrated spheroid. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. There is a faint hint of redder light extending outwards from the core. There is no discernible spiral structure or distinct dust lanes, although the faint periphery has a slightly grainy texture that may indicate a very low level of star formation. The overall morphology suggests a mature galaxy, consistent with an elliptical classification. There are no obvious signs of recent merger activity or significant tidal disturbances.