The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. Its light profile is smooth, lacking any readily apparent spiral arms or distinct features. The core region shows a brighter concentration of light, suggesting a significant stellar population and possible active galactic nucleus. The galaxy exhibits a color gradient, transitioning from a yellowish core to bluish hues in the outer regions. This color difference might be due to differing stellar populations, where the core is dominated by older, redder stars, while the outer regions may harbor younger, bluer stars due to ongoing or recent star formation. There is a slight hint of possible tidal disturbance visible in the outskirts of the galaxy, implying an ongoing or past interaction with another galaxy. The overall structure indicates an evolved system, with a high likelihood of being an early-type galaxy.
