The galaxy presents a generally smooth and rounded morphology. There is a central, concentrated region that appears brighter with a yellowish hue, gradually fading into an outer halo. While largely smooth, a subtle hint of disk-like structure may be present upon closer inspection, but it is not definitively established based on the image. The galaxy exhibits little indication of significant disturbances or recent major merger events; only a minor disturbance can be seen. The roundness dominates over any elongated or cigar-like appearance. The overall color suggests a population of older stars, possibly with ongoing star formation. The estimated size indicates a substantial physical extent for this galaxy.
