The galaxy presents as a relatively compact, elliptical system. Its overall color profile indicates an older stellar population, with a dominant yellowish-red hue emanating from the central region. The light distribution appears smooth and centrally concentrated, showing little evidence of spiral arms or significant dust lanes. There is a slight elongation, suggesting a shape that deviates marginally from a perfect sphere. No major signs of recent or ongoing mergers are apparent, with the galaxy displaying a generally undisturbed morphology. Faint, diffuse light extends outwards from the central region, gradually fading into the background sky.
