The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, indicating a high density of stars and potentially a supermassive black hole at its center. There appears to be a radial gradient in the luminosity, decreasing outwards from the core. There is a slight yellowish hue concentrated in the center, gradually transitioning towards redder tones in the outer regions of the galaxy. There is no discernible spiral structure or prominent dust lanes. The galaxy exhibits a symmetrical and compact morphology, appearing undisturbed by any major recent merger events.
