This galaxy appears to be relatively compact, with an overall elliptical shape. The central region exhibits a bright, concentrated core with a bluish hue. This suggests the presence of a population of younger, hotter stars or an active galactic nucleus.

Moving outward from the core, there's a transition to a more yellowish-orange color, possibly indicating an older stellar population. There is a diffuse, extended tail-like structure emanating from the central region towards the top of the image. This may suggest a tidal interaction or recent merger event. Faint hints of disrupted structures or arm-like features are present within the main body of the galaxy. The overall impression is one of a galaxy that has undergone some gravitational disturbance, potentially involving a minor merger with a smaller companion galaxy.
