The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration of light.  It exhibits a subtle color gradient, transitioning from a yellow-white core to a slightly redder outer halo. The overall form is neither perfectly circular nor highly elongated, appearing to be intermediate in shape.  No distinct spiral arm structures or prominent dust lanes are apparent.  There is no obvious sign of ongoing major mergers or significant tidal disturbances, although a very slight asymmetry in the outer halo is possibly present, suggesting the potential for a minor interaction. The galaxy’s overall smoothness indicates a well-mixed stellar population, likely dominated by older stars. Its estimated size is roughly 4 kpc.
