The galaxy presents a largely smooth and centrally concentrated morphology. The core exhibits a yellowish hue, potentially indicative of an older stellar population and lower levels of on-going star formation. The outer regions of the galaxy show a subtle fading in intensity, transitioning to a slightly bluer color. This suggests a population of younger, hotter stars may be present in the galaxy's outer edges. The overall shape appears somewhat elliptical, displaying moderate flattening. There is no obvious sign of strong tidal features or major disturbances, suggesting it is in a relatively quiescent state, although there is a slight lopsidedness in the outer regions.
