The galaxy appears as a relatively smooth, centrally concentrated object with a slight ellipticity. It exhibits a color gradient, appearing bluer in the central regions and redder towards the outer edges. There is no evidence of spiral arms or a prominent disk structure. Minor disturbances might be present, but are not obvious. The overall morphology suggests a relatively evolved system, potentially an elliptical or S0 galaxy, viewed at a distance where finer details are blurred. The light distribution is centrally concentrated and decreases gradually with increasing radius, showing no sharp edges or breaks. The estimated size suggests it is an intermediate-sized galaxy, and its redshift indicates that the galaxy is located at a significant cosmological distance. The rate of star formation may be low within the galaxy. There does not appear to be any mergers or interactions occurring.
