The galaxy presents an overall elliptical morphology. The central region exhibits a high surface brightness, indicating a dense stellar population, likely an older population with a yellow-white hue. The galaxy displays a gradual decline in surface brightness moving outward from the core. There is some evidence of a very faint, diffuse disk structure. There may be signs of a minor disturbance in the structure of the galaxy, but is otherwise a relatively relaxed object with no prominent tidal tails or obvious signs of a major merger. Star formation is likely low, and if it is present, it is constrained to the central portion of the galaxy. 
