The galaxy appears as a centrally concentrated, elliptical structure with a smooth overall morphology. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outwards from the center, the color transitions to a more reddish tone in the outer regions, possibly indicating the presence of dust or a slightly younger population of stars in the galactic periphery. There is little evidence of spiral arms or prominent star-forming regions. The axial ratio implies a somewhat flattened shape, but not a highly elongated or disk-dominated form. Subtle irregularities or minor disturbances may be present in the outer regions.