This galaxy appears to be a spiral, though its structure is somewhat disturbed. It has a moderate redshift, indicating that it is relatively distant. The galaxy possesses a central bulge with spiral arms emanating from it. These arms are not well-defined, suggesting that they might be undergoing some form of disruption. The color distribution indicates that it is relatively massive and has a fairly low rate of star formation. There are indications of potential minor tidal disturbances. The light is dominated by yellow hues.
