The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness, showing minimal disk-like features. The core region displays a strong concentration of light, suggesting the presence of a significant stellar population, possibly an older bulge. The light gradually fades from the center outward, implying a lack of significant spiral arm structure or active star-forming regions across the galaxy's extent. No signs of major disturbances, tidal tails, or interacting companions are apparent in this image, indicating it is likely an isolated and undisturbed system. The galaxy's color profile is slightly redder than the average spiral galaxy, indicative of an older stellar population and a relatively low ongoing star formation rate. The estimated physical size, derived from observed angular diameter at its redshift, suggests this is a reasonably large galaxy.
