The galaxy presents a largely smooth morphology, appearing as a fairly round, concentrated object. The central region exhibits a brighter, yellowish hue, suggesting a population of older stars. There is very little evidence of spiral arm structure. The outer regions of the galaxy are fainter and have a slightly bluer color, possibly indicative of some ongoing, albeit low, star formation. There is a small hint of possible tidal disturbance or minor interaction occurring on the side of the galaxy. The galaxy appears relatively isolated.
