The galaxy presents as a somewhat elongated, disk-like structure. Its color profile is centrally concentrated with a yellowish-white hue, transitioning into a bluish, diffuse outer region. This may indicate a relatively older stellar population in the galactic center. The galaxy appears mostly smooth with a notable lack of distinct spiral arm structures. There may be some subtle evidence of a disk, as some faint features are possibly distinguishable near the edge of the galaxy. The overall structure suggests a generally well-defined but unperturbed morphology.
