The galaxy presents a generally smooth and elliptical morphology. It appears to have a concentrated central bulge, characterized by a yellowish-orange hue, which suggests an older stellar population dominated by redder stars. The outer regions of the galaxy exhibit a fainter and slightly bluer color, hinting at the presence of some ongoing, although likely subdued, star formation activity. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy seems relatively undisturbed, with no prominent tidal features or signs of a major merger event. Its overall appearance suggests a galaxy that is transitioning or has already transitioned to a more quiescent state. The elongated shape could indicate it is an elliptical galaxy with some degree of flattening.
