The galaxy appears as a relatively smooth and rounded object. It exhibits a central concentration of light, with a gradual decrease in brightness outwards. The core of the galaxy shows a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy are fainter and display a subtle reddish tint, potentially indicating the presence of dust or a population of cooler, redder stars. There is a slight asymmetry or possible disturbance on one side of the galaxy, which could be evidence of a minor interaction or recent accretion event. Overall, the galaxy presents as a mature system, with a largely quiescent star formation history.
