The galaxy appears to be an elliptical type. The light distribution suggests a relatively smooth morphology with a concentrated central bulge that dominates the overall light profile. There is little evidence of spiral arms or distinct features such as dust lanes. The central region exhibits a yellowish-orange hue, possibly indicative of an older stellar population, while a hint of blueish-green is visible around the edges, implying a younger, hotter stellar population in those areas. The galaxy exhibits a roughly circular shape, with a slight possibility of minor disturbances in its symmetry. Overall, the galaxy presents a compact and relatively undisturbed structure.
