The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, indicative of an older stellar population. The dominant color is yellowish-orange, suggesting a lack of significant ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. The overall morphology suggests a galaxy that is undergoing passive evolution, and appears to be quite round in shape. There is no apparent evidence of any major merger events in its recent history, although some minor disturbance is possible.
