The galaxy appears as a single, relatively smooth object. There is a concentrated central region which fades gradually outward. The overall shape appears generally elliptical, tending towards round but not perfectly so. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy's color profile indicates a mix of stellar populations, appearing yellowish overall, suggesting the presence of intermediate-age stars. There is no obvious indication of a recent or ongoing major merger, although a minor disturbance may be present in its morphology. There are no significant dust lanes visible, consistent with a galaxy that has largely ceased active star formation.
