The galaxy presents as a somewhat centrally concentrated object, appearing relatively smooth with a generally round morphology. A subtle bluish tint is visible in some regions, possibly indicating areas of younger star formation. The galaxy exhibits some degree of disturbance in its structure, perhaps hints of a tidal tail or asymmetric arm extending from one side. There is a notable difference in color and brightness between the central region and the outer edges. The core is more luminous with a slightly redder hue, suggesting an older stellar population. The outer regions are fainter.
