The galaxy presents as a lenticular or early-type spiral system, with a smooth, centrally concentrated bulge that dominates its overall luminosity profile. The bulge exhibits a yellowish hue, indicative of an older stellar population. A faint, extended disk is potentially present, seen nearly edge-on, with a subtle blue-ish tint hinting at the presence of some younger stars and potential star formation activity, although very limited. The galaxy appears to be relatively isolated, with no major signs of tidal disturbances or ongoing mergers, but there may be minor morphological disturbances suggesting a past interaction. Its shape is elongated but trending towards round. The presence of a central supermassive black hole is inferred. The estimated mass range indicates a substantial galaxy with a relatively low star formation rate, consistent with its classification as a more evolved system.
