The galaxy presents as a somewhat elongated, elliptical-type system. Its central region exhibits a high degree of luminosity, with a concentrated and bright core. Moving outward from the core, the light diffuses into a more gradual gradient, fading into the surrounding space. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The color profile appears generally uniform, with a subtle shift towards redder hues, especially in the central bulge. No signs of significant tidal disturbances, close companion galaxies, or ongoing major merger events are evident in this image.
