The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The central region appears bright and yellowish-white, suggesting an older stellar population. Moving outward, the color gradient shifts towards a slightly bluer hue in the outer regions, which may indicate the presence of some younger stars or ongoing star formation, albeit at a low rate. There is little evidence of prominent spiral arms or significant dust lanes. The overall shape is somewhat elongated, but not extremely so. The galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger or tidal interactions.
