This galaxy appears to be a relatively smooth, centrally concentrated object, exhibiting a somewhat elliptical morphology. There is a noticeable central bulge that is brighter than the surrounding regions. A faint disc structure is subtly suggested around the central region, and a lack of prominent spiral arms or significant dust lanes indicate that it is likely an early-type spiral galaxy or a lenticular galaxy. No obvious signs of recent major merging events are discernible, though some minor asymmetry hints at possible gravitational interaction in the past. The color is generally pale blue, suggesting the presence of some relatively young stellar populations. There are no obvious signs of active star formation.
