The galaxy appears to be a relatively compact object with a bright central region. The morphology is somewhat irregular, with hints of asymmetry in the outer regions. The core exhibits a strong, concentrated luminosity. The galaxy displays a color gradient, with a bluer core transitioning to redder hues in the outer disk. This might indicate a population of younger, hotter stars in the central region and older, cooler stars towards the periphery. There is some indication of possible tidal disturbances or faint features suggestive of minor interactions with another galaxy or recent mergers.
