The galaxy appears to be elliptical in shape, presenting a largely smooth and homogenous structure. It shows a concentrated central bulge that diffuses outwards into a broader, less defined halo. Color gradients are subtle; the core exhibits a yellowish hue, suggesting an older stellar population. Fainter blueish regions are present, but appear as subtle mottling across the body of the galaxy rather than well defined spiral arms or star forming regions. A slight asymmetry is detectable, hinting at a possible minor interaction. The overall appearance suggests a relatively evolved system with subdued star formation activity.
