The galaxy presents as a centrally concentrated object with a generally smooth appearance. The central region is a bright, yellowish-orange hue, suggesting an older stellar population. Moving outward, the light appears to fade and become slightly redder, indicating a possible gradient in stellar populations with potentially younger, bluer stars further from the center, although this is subtle. There are no clear spiral arms or a distinct disk-like structure visible. There is a hint of some irregularity in the outer regions; this could be due to tidal interactions, or internal dynamics, however, the limited resolution makes it difficult to determine the exact cause. Overall, the galaxy appears to be more elliptical or lenticular in shape, dominated by a bulge. A very subtle extension of diffuse light is visible, especially to one side, which might indicate a faint halo or tidal debris. 
