The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, concentrated morphology. Its overall shape is approximately round. The central region displays a bright, yellowish hue, suggesting a population of older stars. Moving outward from the center, the color subtly transitions to a redder tone. There is no visible evidence of spiral arms or significant dust lanes. No major mergers are visibly occurring. The overall appearance indicates a system that is relatively evolved, potentially with a suppressed star formation rate.
