The galaxy presents as an elliptical or lenticular morphology, appearing largely smooth and centrally concentrated. Its overall color is yellowish-white, suggesting an older stellar population with fewer young, hot stars. The isophotes are moderately elongated, displaying a slight deviation from a perfectly circular shape. There are no clearly discernible spiral arms or distinct dust lanes. There is a hint of some interaction to the north of the galaxy. There appears to be a region with a different color/stellar population residing there. No clear signs of ongoing major merger activity are apparent, such as tidal tails or significant distortions in the galaxy's overall structure, but minor disturbances may be possible. Overall, this galaxy likely has a high stellar mass and a low star formation rate.
