The galaxy presents as an elliptical morphology, characterized by a relatively smooth and concentrated light distribution. The galaxy exhibits a noticeable color gradient, transitioning from a bluer hue in the central region to a redder hue in the outer regions. A slight asymmetry is perceptible, potentially indicative of a minor interaction or internal disturbance. No distinct spiral arms or prominent dust lanes are visually apparent. The light distribution suggests an evolved stellar population, particularly in the outer regions. The galaxy appears relatively isolated in its immediate vicinity.
