The galaxy presents as a slightly elongated, elliptical structure. The core exhibits a bright, concentrated luminosity with a yellowish hue, suggesting an older stellar population. Moving outward from the core, the luminosity gradually decreases. The galaxy appears relatively smooth with a lack of distinct spiral arms or prominent dust lanes. There are hints of a disk-like structure, though less defined. The overall color gradient shifts from yellow at the core to a slightly redder tone in the outer regions. The absence of significant irregularities suggests no ongoing major merger events. There are no visual artifacts. 
