The galaxy presents as a relatively smooth, elliptical-like structure, displaying a mostly homogenous light distribution with a slight elongation. The object shows a higher concentration of luminosity in the central region which fades into the surrounding space. The color profile appears to be skewed towards the red end of the spectrum, indicating a population of older stars. There seems to be little evidence of active star formation within the galaxy. The morphology suggests a system that is likely relaxed, without major signs of recent interactions or disturbances.