The galaxy presents a smooth, elliptical morphology, exhibiting a high degree of central concentration. The light distribution appears relatively uniform and lacks prominent spiral arms or distinct features, suggesting an older stellar population. Its color profile shifts from a brighter, yellowish core to slightly redder hues in the outer regions. There are no discernible signs of recent major merger activity. The galaxy has an estimated effective radius of a few kiloparsecs. The moderate redshift indicates a considerable distance, influencing the observed properties such as apparent size and luminosity. The galaxy appears to be undergoing a relatively low rate of star formation.
