The observed galaxy presents a roughly elliptical morphology. There appears to be a bright, concentrated central region that gradually fades towards the outer edges of the galaxy. The color profile indicates a blue-white hue at the core, transitioning to green and finally a blue-reddish tone at the outer edges. This may suggest varying stellar populations, with potentially younger, hotter stars dominating the central region and older populations residing in the outer parts. No distinct spiral arm structures or bar features are immediately apparent. There are subtle, potential signs of minor disturbances in the shape and color distribution.
