The galaxy presents as an elliptical morphology with a smooth, diffuse light profile. The central region exhibits a brighter, more concentrated luminosity. The overall color appears to be reddish-yellow, which could indicate an older stellar population and lower current star formation activity. The galaxy's shape is elongated, tending toward a cigar-like shape, and exhibits no obvious spiral arm structures or significant dust lanes. There is no indication of a major ongoing merger event, though some minor asymmetry might suggest past interaction.
