The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction. The primary structure appears relatively smooth and somewhat rounded, with a central concentration of luminosity. 

There's evidence of possible tidal features or distortions extending from the main body. A secondary, less defined component is observed, suggestive of a potential companion galaxy or a disrupted region within the primary galaxy itself. There is possible evidence of a minor disturbance and merger, although an artifact cannot be ruled out.

Color variations are present across the galaxy. The central region exhibits a bluer hue, possibly reflecting recent or ongoing star formation activity. Fainter, redder areas are also apparent which could be evidence of an aging stellar population. The overall light profile appears to be somewhat diffuse.
