The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears elliptical, exhibiting a radial decrease in surface brightness from the core outwards. The core region appears to have a reddish hue, which could indicate an older stellar population. Moving outward, the surrounding halo takes on a bluish tint. The overall structure of the galaxy lacks significant disturbances or asymmetries, suggesting it has not undergone a major merger recently. The size suggests this is a relatively small galaxy. The morphology implies it's likely a galaxy with low star formation activity.
