The galaxy presents an overall smooth morphology, with a roughly elliptical shape. The light distribution appears concentrated toward the center, suggesting a prominent bulge component. Faint extended features are visible emanating from the central region. The galaxy exhibits a color gradient, transitioning from bluer hues in the inner regions to redder hues in the outer regions. The color variation could indicate differing stellar populations or dust content throughout the galaxy. There is indication of a potential minor disturbance in the galaxy's morphology and asymmetry that suggests possible past interaction with another object.
