The galaxy presents an elliptical morphology with a high degree of central concentration, indicated by the bright central bulge. The light distribution appears relatively smooth, suggesting a lack of significant recent major merger events. The disk is clearly visible around the bulge, appearing as a haze of gas surrounding it. The bluer color in the disk indicates the presence of younger stars. The color gradients suggest a population of older stars in the bulge, shifting to younger stars in the outer disk. There appears to be a small, nearly insignificant dust lane bisecting the disk, potentially obscuring some of the light. There is some evidence of disturbance, potentially from a minor merger, indicating the presence of tidal tails. It has spiral arms as well. Overall, it appears to be an intermediate galaxy between a spiral galaxy and an elliptical galaxy.
