The galaxy in question presents a generally smooth morphology. The light is concentrated towards the center, indicating a prominent bulge. Its overall shape appears somewhat elliptical, although not perfectly so. There is a slight elongation, but it is not highly elongated. There are some suggestions of disturbances in the galaxy's outer regions, though they are not overtly pronounced. The disturbances could potentially be evidence of a past or ongoing minor interaction with another galaxy. The galaxy's color is yellowish-white, which is indicative of a stellar population that is neither exceptionally young nor particularly old. Its estimated size is around 4.6 kpc, which is not a particularly large galaxy. The estimated redshift suggests that it is a fairly distant object. Overall, the galaxy looks to be an intermediate-mass galaxy with an intermediate age stellar population and some signs of possible past interactions. 
