The observed galaxy presents as a relatively smooth, flattened elliptical morphology. There is a noticeable central bulge that appears brighter and more concentrated than the surrounding disk. The disk shows a faint, bluish hue indicating the potential presence of young stars and ongoing, albeit low, star formation. The galaxy exhibits a slight elongation, its overall structure seemingly undisturbed, suggesting it is not currently undergoing a major merging event. The overall light distribution is centrally concentrated, consistent with a high Sersic index.
