The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. It demonstrates a high degree of central concentration, with light intensity diminishing gradually outward from the core. Its shape is largely round, with a near absence of any visible spiral arm structure or disk-like component. There is no apparent ongoing major merging activity or significant tidal disturbances, but there is some indication of a possible minor disturbance or interaction. The galaxy exhibits a moderate redshift, suggesting it is at an intermediate cosmological distance. The color profile indicates the presence of an aging stellar population. Overall, the galaxy appears as a relatively passive and evolved system.
