The galaxy presents as a somewhat elongated structure. Its overall color profile tends toward the redder end of the spectrum, with the presence of some regions showing slight bluer tones, especially around the periphery of one side. The central region appears brighter and more concentrated. The galaxy exhibits a relatively smooth appearance with some possible faint features indicating either spiral arms or tidal disruptions due to an ongoing or past interaction, but its shape is largely amorphous. The system appears relatively isolated, with no obvious indications of a major merger in progress, however there could be a minor merging event.
