The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It exhibits a roughly circular shape, with a concentrated central bulge. The light distribution suggests an elliptical galaxy, potentially of the E0-E3 subtype. The galaxy is dominated by light in the redder bands suggesting an older stellar population. There are hints of bluer light in the surrounding region, but no well-defined spiral arms or disk structure are clearly visible in this image. The overall color suggests intermediate to high mass range, with a moderate rate of star formation. There is no evidence of major ongoing mergers or significant tidal disturbances based on the morphology, with only minor disturbances at most.
