The galaxy presents an overall elliptical morphology, appearing largely smooth in structure, but with some disk-like qualities. It exhibits a concentrated central region with decreasing luminosity towards its outer edges. There is a slight elongation, but it appears generally rounded. Color gradients are subtle, with a bluer hue in the central regions possibly indicating recent star formation, with the color of the galaxy becoming redder towards the periphery, potentially indicative of an older stellar population. No strong evidence of spiral arms or a prominent bar structure is readily apparent in this image. There is a possible slight disturbance in the structure, but no strong indications of ongoing major merger activity. The overall light distribution suggests a system that is neither perfectly smooth, nor heavily disturbed.
