The galaxy presents a smooth, elliptical morphology, exhibiting a concentrated central bulge. The light profile appears relatively uniform, with a gradual decrease in intensity from the core outwards. The color is predominantly yellow-orange, suggesting an older stellar population with limited ongoing star formation. There are subtle hints of bluer regions at the periphery, possibly indicating the presence of younger, hotter stars, albeit at a low level. There is no clear evidence of spiral arms or a distinct disk structure. The overall impression is of a mature, quiescent galaxy with a small amount of disturbance in its shape.
