The galaxy presents as a largely featureless, elliptical-like system. It exhibits a centrally concentrated luminosity profile, with a smooth, gradual decline in surface brightness from the core outwards. The core region appears bright and relatively compact, indicative of a high stellar density. The overall color is generally blue, but it lacks resolved spiral arms or prominent dust lanes. There is no noticeable disturbance to its structure. The galaxy appears relatively isolated. There are signs that some star formation may be occuring, although not at a very high rate. 
