This galaxy appears as a somewhat disturbed system, possibly undergoing a merging event. It presents an overall elliptical shape with a smooth central concentration of light, suggesting a well-established spheroidal component. The galaxy exhibits a yellowish-red hue in the center, which may indicate an older stellar population. There are two distinct bright areas which could represent the two separate components of the merging galaxy. A faint bluish extension is observed on the edge of the galaxy, potentially indicative of ongoing star formation, although it could also be tidal debris resulting from the interaction. Given the disturbed morphology, the galaxy does not appear to be a simple elliptical, but rather a system in transition. Further spectroscopic observations are required to fully understand the dynamics and star formation history of this object.
