The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution with a high degree of central concentration. The overall color is yellowish-orange, indicative of an older stellar population and a lack of significant ongoing star formation. There are no visible spiral arm structures or prominent dust lanes. The galaxy appears relatively isolated with potentially some minor disturbances, suggesting a possible past interaction or minor merger event, although a single, well-defined nucleus is still present. The galaxy’s shape is generally round, deviating slightly towards an intermediate form. Overall, this object is consistent with a massive elliptical galaxy at a moderate distance.
