The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution suggests a primarily spheroidal structure, exhibiting little to no discernible disk component. The core of the galaxy presents a bright, yellowish hue, possibly indicating an older stellar population dominating the central region. Fainter, reddish-tinged light extends outwards from the core, gradually diminishing in intensity. There's no strong evidence of spiral arms or significant dust lanes. Overall, the galaxy presents as a well-defined, relatively undisturbed system, suggesting a lack of recent major merger events.
