The galaxy presents a generally smooth morphology, appearing largely featureless with a high degree of central concentration. Its shape is approximately round, deviating slightly from a perfect circle. There is a subtle color gradient, transitioning from a yellow-orange hue at the core to a redder color towards the outer regions. No prominent spiral arms or distinct dust lanes are visible. The overall structure suggests an evolved system, possibly with a significant population of older stars and a low rate of on-going star formation. There is no obvious visual evidence of recent or ongoing major merger activity. Any disturbances appear to be minor, if present.
