The galaxy appears as a relatively compact and centrally concentrated object. It presents a generally smooth morphology, although subtle variations in color and brightness suggest the presence of some internal structure. The galaxy's color profile indicates a redder hue overall, particularly toward the central region, transitioning to slightly bluer tones in the outer regions. This color variation could indicate varying stellar populations, with older, redder stars dominating the core and younger, bluer stars present in the outer regions, with the possibility of ongoing, low-level star formation. 

There is a hint of asymmetry and minor disturbances present in the galaxy's morphology. A slight elongation or distortion is visible, suggesting the possibility of a past interaction or merger event. The bulk of the galaxy appears well-defined, and without strong evidence for a major interaction, it is most likely that it is experiencing internal processes. 
