The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. There may be a slight hint of disk-like structure, but this is not obvious. There appears to be a very mild disturbance within the galaxy, based on a small amount of visual asymmetry. The galaxy’s core exhibits a yellowish hue, suggesting an older stellar population, while outer regions possess a bluer tint, indicating ongoing or recent star formation. The galaxy is generally round, but not completely so. It's luminosity suggests it is a relatively massive galaxy.
