The galaxy presents as a largely smooth structure, appearing elliptical in shape. There is a concentrated central bulge exhibiting a yellowish-orange hue, indicating an older stellar population. This core region appears to dominate the overall light output of the galaxy. Fainter, bluer extensions are subtle, suggesting a possible presence of ongoing, albeit limited, star formation in the outer regions. The overall color profile suggests a mature galaxy with a mix of old and potentially a small population of young stars. The morphology displays a lack of prominent spiral arms or significant dust lanes.
