The galaxy presents an elliptical morphology, appearing elongated with a smooth, diffuse profile. A bright central bulge dominates the structure, with the light intensity decreasing gradually towards the outer edges. There is a slight color gradient observed, transitioning from a yellow-white core to a subtly bluer halo, possibly indicating variations in stellar populations. No distinct spiral arms or prominent dust lanes are discernible within the observed image. The overall structure suggests a relatively evolved system, potentially with a significant population of older stars. A hint of possible tidal disturbance is visible in the outer edges of the halo, but is not very obvious.
