The galaxy presents a generally smooth and centrally concentrated appearance. Its shape is neither perfectly spherical nor highly elongated, suggesting an intermediate ellipticity. The color distribution within the galaxy shows a noticeable gradient, transitioning from a more yellowish hue in the central regions to a redder tint in the outer areas. The relative color distribution may indicate older stellar populations. There are faint indications of potentially disturbed morphology, possibly resulting from minor gravitational interactions. There is also a blue-green color on the left side which may indicate an area of star formation. It is also possible that this object is the result of two galaxies merging.
