The galaxy appears to be an elliptical type, exhibiting a generally smooth, concentrated morphology. Its shape is largely spheroidal. The core region presents a yellowish-white hue, suggesting an older stellar population. There is a notable absence of prominent spiral arms or a defined disk structure. No significant signs of on-going mergers or major disturbances are visible in this image. The light appears relatively uniform across the galaxy's surface, lacking the patchy, uneven distribution that would be indicative of active star formation regions.
