The galaxy appears relatively compact with a bright, concentrated central region. There is evidence of bluer color in the central part, which may indicate recent star formation or an active galactic nucleus. The outskirts of the galaxy are fainter and display a slightly redder hue. The overall morphology appears largely smooth with only slight irregularities suggesting the possibility of minor disturbances or a recent merger event. However, the smoothness suggests that such events may be in the distant past. There is no strong presence of spiral arms or a well-defined disk. Overall, this seems to be a galaxy which is generally smooth in appearance, with some minor irregularities suggesting the potential for past interactions.
