The galaxy appears to be a relatively smooth, elliptical galaxy with a prominent bulge. The core exhibits a concentrated, bright yellow-orange hue, suggesting a population of older stars. There may be a slight hint of a disk feature, visible as a faint, extended tail, or tidal stream. There is no evidence of a recent major merger, though there may be minor disturbances that can't be fully seen in this image. Based on the color profile, star formation is likely minimal or non-existent at present. The overall roundness indicates the system is largely relaxed and undisturbed, representing a later stage in galactic evolution.
