The galaxy presents as a likely elliptical or lenticular morphology, exhibiting a smooth, featureless structure. The light profile appears concentrated towards the center, indicating a high degree of central mass concentration. There is a possible merging event that could be occurring. The galaxy has what appears to be a double nucleus, which suggest a possible ongoing or recent merger with another galaxy of non-negligible size. The primary body of the galaxy displays a yellowish-orange color, possibly indicative of an older stellar population and a low rate of star formation. The galaxy appears relatively round in shape, with no strong indications of a significant disk structure. The observed features suggest a massive galaxy, undergoing or having undergone significant gravitational interaction, and with a quiescent star formation history.
