The galaxy presents a largely smooth morphology, with a dominant spheroidal component. There is a slight asymmetry, but no obvious spiral arm structure is visible. The galaxy is fairly round. Color gradients are present; the central region appears more white, suggesting a population of older stars, while the outer regions exhibit a bluer tint, possibly indicative of ongoing, or more recent star formation. There is a neighboring small, bright object to the right. A significant portion of the galaxy's population appears to be older, and there is a notable amount of star formation occurring.
