This galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth, relatively featureless profile, suggesting an older stellar population. The color gradient transitions from a bright, yellowish core to a slightly bluer outer halo. There is no obvious spiral arm structure or prominent dust lanes visible. The galaxy appears relatively isolated, with no signs of major tidal disturbance or ongoing merger activity, although there may be some minor perturbation or weak interaction. Overall, it presents as a relatively evolved system.
