The galaxy presents as an elliptical object with a somewhat disturbed morphology, hinting at possible past or ongoing interactions. There is no distinct spiral structure observed. The galaxy's light profile appears relatively smooth overall but has some non-uniform distributions within its central region. Specifically, there are some minor disruptions suggesting a more complex, possibly merging or interacting system. There appear to be two main dense regions suggesting it could be in the early stages of a merger. There's a color gradient observable from the central region extending outward, though it's not particularly pronounced, indicating some level of ongoing or recent star formation activity. The overall color of the galaxy appears to be a slightly yellowish or reddish tint, indicating an older stellar population with potentially suppressed recent or ongoing star formation.
