The galaxy presents as a centrally concentrated system with a generally smooth morphology. The core exhibits a bright, yellowish-orange hue, suggesting a significant population of older stars. Moving outward from the core, the color transitions to a slightly greener shade, possibly indicating the presence of a younger stellar population, or regions of low-level star formation. The galaxy lacks distinct spiral arm structures or a well-defined disk. There is no sign of major mergers, but a minor disturbance or some interaction cannot be completely ruled out. Overall, the galaxy appears to be relatively undisturbed, showing a morphology consistent with an elliptical or lenticular galaxy.
