The galaxy presents as a luminous, centrally concentrated object, exhibiting a generally smooth morphology. There is an apparent lack of distinct spiral arm structures or prominent dust lanes within the visible portion of the galaxy. The radial light profile suggests that the galaxy is largely spheroidal in shape with the concentration of light appearing at the center. The galaxy appears roughly circular or elliptical. Faint disturbances hint at possible past minor interactions. The dominant color of the galaxy is a yellowish hue, suggesting an older stellar population. Overall, the morphology is indicative of an elliptical galaxy with a red-sequence stellar population and negligible ongoing star formation.
