The galaxy presents as a somewhat elongated, disk-like structure, possibly exhibiting characteristics of an elliptical galaxy. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The disk component, while present, is relatively faint and blends smoothly into the surrounding space. A slight color gradient exists, transitioning from the yellowish core to fainter, redder edges, which may indicate a radial variation in stellar populations or dust content. There appears to be a lack of distinct spiral arm structures. The overall morphology suggests a galaxy that has largely ceased significant star formation.
