The galaxy appears as a singular, fairly homogenous entity. It exhibits a generally elliptical morphology, showing a high degree of roundness. There is a smooth, bright central concentration of light, suggesting a substantial galactic nucleus. The color profile appears relatively uniform across the galaxy, with a slight reddening toward the outer edges. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy’s light distribution is primarily smooth, indicating a lack of significant star formation activity. The overall structure suggests a system that is largely undisturbed. There are no prominent tidal tails, bridges, or signs of ongoing or recent merger events, supporting the notion of a galaxy at relative rest. Based on its color and morphology, this galaxy may be composed primarily of older stellar populations.
