This galaxy presents a generally smooth morphology, with a centrally concentrated, roughly elliptical light distribution. The core exhibits a yellow-orange hue, suggesting a population of older stars. There is a subtle color gradient from the core to the outer regions, with the periphery appearing slightly bluer. This bluer color suggests the presence of a younger stellar population compared to the core. No distinct spiral arms or prominent dust lanes are visible, indicating a relatively undisturbed structure. The galaxy's shape is more 'in between' a circle and an elongated ellipse rather than either extreme. There is no obvious indication of tidal tails, major mergers, or significant disturbances in its structure, though there is a faint hint of a minor disturbance.
