The galaxy presents as a largely featureless, elliptical-like system with a high degree of central concentration. It exhibits a smooth, diffuse light profile, transitioning gradually from a bright, yellowish core to fainter, redder outskirts. There is a very subtle, almost imperceptible elongation, deviating slightly from a perfectly circular shape. No distinct spiral arms or dust lanes are visible. The color gradient suggests a stellar population that is older and less actively forming stars, with a small population of young stars forming. There is no evidence of significant tidal disturbances or ongoing mergers, indicating a relatively isolated and undisturbed evolutionary history. Overall, the object appears to be a quiescent, early-type galaxy.
