The galaxy presents a primarily smooth morphology, with a concentrated central bulge that exhibits a yellowish hue, indicative of an older stellar population. This suggests a lower rate of ongoing star formation in the nuclear region. Faint, bluer extensions emanate from the core, hinting at regions with younger stars or perhaps ongoing star formation. These extensions are not well-defined as spiral arms, but suggest some level of disk-like structure. There is an indication of a slight disturbance in the overall structure. The galaxy displays an intermediate degree of roundness. Overall, the light distribution appears relatively smooth and centrally concentrated.
