The galaxy appears to be an elliptical type. It exhibits a centrally concentrated luminosity profile, with the brightest region located in the core. There is a smooth transition of light intensity from the center outwards, with no distinct features like spiral arms or a bar structure visible. The overall shape of the galaxy is somewhat elongated. The color profile suggests a relatively old stellar population, with a dominant yellow to red hue in the central region. Fainter blue light is present at the periphery. A smooth, even distribution of light indicates minimal dust obscuration.
