The galaxy presents as a fairly smooth, elliptical structure with a high degree of central concentration. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central regions. There is a slight elongation, implying a deviation from a perfect sphere, leaning more towards a flattened spheroidal shape. No distinct spiral arms or significant dust lanes are readily apparent in the image. The overall morphology is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy, with no major disturbances or signs of recent merger activity visible. The outskirts appear to fade gradually into the background, indicating a lack of sharp edges or distinct features beyond the main body.
