The galaxy appears as a single, relatively smooth object with no distinct spiral arm structures or significant dust lanes visible. The light distribution suggests an elliptical morphology, with a highly concentrated core region that gradually fades into the outer regions. The color gradient indicates a yellowish core, potentially indicative of an older stellar population and reduced star formation activity in the central region. The overall appearance of the galaxy is undisturbed, with no signs of recent major merger events or significant tidal interactions. The lack of prominent features suggests a lack of ongoing, intense star formation. The galaxy appears relatively isolated.
