The galaxy presents a predominantly smooth morphology, with a notable absence of distinct spiral arms or other prominent features. The light distribution is concentrated towards the center, indicating a bulge component. The galaxy is elliptical in shape, appearing elongated along one axis, though not extremely so. The color gradient suggests a population of older stars dominating the light output, giving it a yellowish hue. There is no strong evidence of active star formation discernible in this image. There is no prominent disk. No signs of tidal tails or major distortions are visible, suggesting it is not undergoing a major merger, although there is a hint of slight asymmetry on one side.
