The galaxy presents as a relatively smooth, amorphous structure with a concentrated central bulge exhibiting a yellowish-orange hue. There is a suggestion of a disk component, although it lacks well-defined spiral arms. A faint, bluish extension appears to protrude from one side of the central region, hinting at a possible tidal feature or interaction with a smaller companion. The overall shape is somewhat irregular, deviating from a perfect elliptical or spiral form. The galaxy's moderate redshift indicates it is at a significant cosmological distance. The colors present are dominated by older stellar populations, though there is possible evidence of ongoing, but limited, star formation in the bluer region. The galaxy has a moderate mass. There is evidence of a potential ongoing merger.
