The galaxy presents a relatively smooth, elliptical morphology. It appears largely featureless with a centrally concentrated bulge. The light is predominantly yellow/gold, suggesting an older stellar population. There is a notable absence of distinct spiral arms or significant dust lanes. The galaxy exhibits a high degree of roundness, with minimal distortion or elongation. There is no evidence of ongoing mergers or tidal disturbances. The galaxy likely has a supermassive black hole at the center and a very old stellar population. Star formation is likely suppressed.
