The galaxy presents a generally smooth appearance with a slight central concentration of light. It exhibits an overall rounded morphology, though not perfectly spherical. There is evidence of some disturbed features and potential interactions within the system, including a plume or tidal tail, indicative of possible mergers. The galaxy displays a color gradient, becoming bluer in the outskirts and more reddish in the center. The blue color suggests the presence of younger, hotter stars, potentially indicative of active star formation regions in the surrounding region. There appears to be one primary component, surrounded by smaller, more diffuse components. The galaxy seems to have undergone some sort of disturbance in its past, although it is not currently in the process of a major merger. 
