The galaxy appears as a relatively smooth, elliptical object. Its light profile exhibits a centrally concentrated luminosity, gradually decreasing towards the outer regions. The color is predominantly a warm yellow-orange hue, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The morphology indicates a galaxy with a high degree of sphericity, with no apparent signs of major mergers or tidal disturbances in the immediate vicinity. Faint, diffuse extensions may exist at the outskirts, but are not clearly defined.
