The galaxy presents as a luminous, elliptical-shaped object. Its color profile indicates a dominance of older stellar populations, exhibiting a reddish-orange hue. The light is smoothly distributed, suggesting a relatively even density of stars within its structure. The galaxy appears elongated, leaning toward a cigar-shaped morphology. There is no discernible spiral structure or prominent dust lanes. Minor disturbances may be present, indicating a possible interaction or past merger event. Overall, the galaxy appears as a mature, relatively quiescent system, potentially hosting a significant population of red giant stars.
