The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. The luminosity appears highest in the central region, gradually decreasing towards the outer edges. A subtle color gradient is observed, with a hint of bluer hues in the surrounding regions and yellow and red-shifted color in the inner bulge. This color variation could indicate ongoing, or recent, star formation in the outer parts relative to the older stellar populations in the galactic center. The galaxy exhibits some dust lanes or features, although they are not distinct or heavily obscuring, which may be due to tidal interactions. The overall shape is somewhat elongated, but not dramatically so.
