The galaxy presents as a fairly symmetrical, elliptical morphology. The light distribution appears smooth and centrally concentrated, with a gradual decline in brightness from the core outwards. There is no discernible spiral arm structure or prominent dust lane. The color profile suggests a relatively old stellar population, dominated by redder wavelengths, which can be seen in the inner and higher density regions. The absence of blue regions indicates a low star formation rate. There is a slight visual elongation in the galaxy's shape. Overall, this galaxy presents as a relatively evolved system without significant ongoing mergers or star formation.
