The galaxy presents a generally smooth, elliptical morphology. It is elongated in shape, with a noticeable bulge at its center. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color profile indicates a dominant population of older stars, as evidenced by the yellowish hue. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer, implying the presence of some younger stellar populations, although the overall star formation rate appears subdued. There's no clear evidence of spiral arms or significant dust lanes, suggesting a relatively undisturbed evolutionary history. The overall structure is quite regular, with no major tidal features or obvious signs of recent merger activity, though minor disturbances cannot be ruled out.
