The galaxy presents a largely smooth morphology. The central region exhibits a concentrated, bright yellow color, which may indicate an older stellar population within the galactic bulge. Moving outwards from the center, there's a gradual transition to a less intense bluish halo, suggesting the presence of some younger, bluer stars in the outer regions. There's no obvious spiral structure or distinct features, leading to the classification as a possibly elliptical galaxy, viewed close to face-on. Minor irregularities or disturbances might be present but are not immediately clear given the image resolution, the possibility of faint tidal features cannot be ruled out. Overall, the galaxy appears relatively isolated and undisturbed.
