The galaxy presents a relatively smooth and symmetrical appearance. It has a generally elliptical morphology, appearing quite round. There is a concentrated central bulge that is bright yellow, possibly indicative of an older stellar population. The luminosity fades gradually toward the outer edges of the galaxy, with no distinct spiral arm structures or prominent dust lanes visible. There are no other galaxies nearby that would indicate a merger is actively occuring. Some faint disturbances are visible, but are minor in comparison to the size of the galaxy. The galaxy's color suggests moderate redshift.
