The galaxy exhibits a predominantly red hue, suggesting an older stellar population and/or significant dust obscuration. The morphology appears relatively smooth and compact, with no discernible spiral arms or bar structure. There is some evidence of minor asymmetry or a slight tidal feature, possibly indicating a past or ongoing interaction with another galaxy, although the overall structure is relatively undisturbed. The galaxy is small and faint. The color difference between the r and z bands suggest that the object is likely a high redshift galaxy.
