The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The central region displays a bright, yellowish-white hue, potentially indicating an older stellar population. The galaxy's overall shape is elongated, but appears closer to round, lacking a strong disk-like structure. Faint extensions of light are present, with one distinct extension on its side. There's little evidence of active star formation regions or spiral arm structures within the visible spectrum. There's no obvious signs of an ongoing major merger event. The overall appearance suggests a galaxy dominated by evolved stars with limited ongoing star formation.
