The galaxy presents an overall smooth appearance, with a degree of elongation along its major axis suggesting an elliptical morphology or a disk galaxy viewed at an angle. There is a slightly brighter, more defined central region, indicative of a galactic bulge. The color gradient across the galaxy appears subtle, with a possible slight bluer tinge towards the edges, hinting at potential younger stellar populations in the outer regions. There appears to be a potential tidal tail or distorted structure in the surrounding space. This could imply a past or ongoing interaction with another galaxy. There is no indication of active star formation regions. Given the estimated redshift, this galaxy is at a substantial distance.
