The galaxy appears as a somewhat amorphous, moderately concentrated object. The central region exhibits a relatively smooth, diffuse glow, transitioning outward to a less defined halo. The overall color profile suggests a mix of stellar populations, with a hint of younger, bluer stars intermixed with older, redder components. There is a significant degree of disturbance with evidence of some interaction and merger events. The morphological classification indicates that the galaxy does not exhibit strong spiral arm features or a well-defined disk structure. It appears to be an elliptical-like galaxy with disturbed features, possibly the result of an ongoing or recent merger.
