The galaxy presents as a somewhat smooth and elliptical object, exhibiting a moderate concentration of light towards its center. The radial light profile appears to decrease gradually from the core outwards, with no obvious spiral arm structures visible in this image. The galaxy appears to have a yellow hue, potentially indicating an older stellar population, and a relatively low rate of ongoing star formation. The morphology is indicative of a system that is not currently undergoing any major merger events, though subtle disturbances may be present. It has an elongated shape, as it is significantly longer than it is wide.
