The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular type. The galaxy exhibits a slightly elongated shape. Color gradients are subtle, with a possible trend towards redder hues in the central region compared to the outer parts. The overall color suggests a population of older stars, with a low current star formation rate. No obvious spiral arms or significant dust lanes are observed. There's a lack of tidal tails or any other disturbances, which points to the galaxy not having undergone a recent major merger event.
