The galaxy presents an overall elliptical morphology, though with subtle features suggesting the presence of a disk component. The central region exhibits a high surface brightness, appearing smooth and concentrated. The color is suggestive of an older stellar population. Proceeding outwards, the brightness diminishes gradually. The galaxy exhibits a slight bluing, especially at the outer regions, which could be indicative of younger stars within a more evolved galaxy. There's a suggestion of disturbed morphology, possibly due to a minor interaction or past merger event, though this is uncertain due to the limited resolution of the image. Overall, the galaxy appears to be in a relatively quiescent state, and the estimated size and shape are representative of an intermediate-sized galaxy.
