The galaxy presents a largely smooth morphology, characterized by a high degree of central concentration. It appears nearly circular, with a radial profile that suggests minimal disturbance. A slight color gradient is observed, with the central region exhibiting a more yellow hue and a gradual transition to a bluer periphery. Based on the color profile, it exhibits some active star formation. There are no obvious spiral arms, bars, or tidal features, suggesting that it is not currently undergoing a major merger.
