The galaxy presents an elliptical morphology, appearing generally smooth in structure without prominent spiral arms or a distinct disk. Its light is concentrated towards the center, suggesting a high degree of central mass concentration. The galaxy exhibits a moderate ellipticity. Its light profile appears well-fit by a Sersic profile with a relatively high Sersic index, further supporting its elliptical classification. The galaxy exhibits a redder color, indicative of an older stellar population and a lower rate of on-going star formation. It is likely a massive galaxy. No signs of active galactic nuclei activity are apparent from the image alone. There are no obvious signs of interactions or mergers.
