The galaxy appears as a diffuse, elliptical-like structure with a high degree of central concentration. A bright, unresolved core dominates the central region, suggesting the presence of a supermassive black hole and/or a dense concentration of stars. The light profile fades gradually from the core outwards. The main body of the galaxy exhibits a relatively smooth texture, showing no prominent spiral arms or dust lanes. The color distribution appears mostly homogeneous, with a slightly bluer hue towards the outer regions. The galaxy displays minimal signs of tidal disturbances or recent merger activity, but faint asymmetry may indicate minor interaction or ongoing accretion.
