This galaxy presents a diffuse, somewhat irregular morphology. The light profile appears centrally concentrated with a smooth, spheroidal component dominating the overall structure, but there is evidence of extended, less-structured features. The core region exhibits a yellowish hue, suggestive of an older stellar population. Faint blue tinges seem to be present throughout a small portion of the galaxy, possibly indicative of more recent, localized star formation. There is a hint of a disturbance in the galaxy shape, possibly due to an ongoing or past merger event; this is seen primarily from the fact that there are two distinct centers to the galaxy. The overall color suggests a galaxy with moderate mass and low star formation rate, with some indications of past or current interactions.
