The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a defined disk structure. The light distribution is centrally concentrated, with a gradual decrease in intensity outwards. The galaxy exhibits a relatively round shape. There is a hint of minor disturbance in the overall symmetry, but no clear signs of ongoing major merger activity. The color profile suggests a mix of stellar populations. A yellowish-orange core possibly indicates an older stellar population, while the surrounding regions contain bluer and more green-toned star formations which could indicate regions of ongoing star formation. The galaxy's overall color is somewhat red.
