The galaxy appears to be an elliptical galaxy, with a relatively smooth and centrally concentrated light distribution. It exhibits a moderate redshift, suggesting a substantial distance. Its apparent shape is somewhat rounded, with a hint of elongation. There is a prominent central bulge, exhibiting a reddish hue, possibly indicative of an older stellar population. A slightly brighter, more intense central region may suggest the presence of an active galactic nucleus or a particularly dense concentration of stars. There is an apparent disturbance in the surrounding region, indicating a potential recent or ongoing interaction or minor merger with another galaxy. The galaxy exhibits a relatively high mass. The star formation rate is relatively low, and the specific star formation rate is especially low, suggesting a quiescent galaxy with minimal ongoing star formation activity.
