The galaxy appears to be a relatively smooth, elliptical-type galaxy, with a high degree of central concentration. It displays a yellowish hue, suggesting an older stellar population and lower levels of current star formation. The galaxy exhibits a generally round morphology, with no obvious features such as spiral arms or a distinct disk component visible in this image. There are no signs of tidal disturbances or ongoing mergers, indicating it is likely a relatively isolated system. The overall light distribution indicates a centrally-dominated system. The apparent size is relatively small, possibly a factor of its distance.
