The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth light distribution. The core region demonstrates a bright, yellowish hue which suggests an older stellar population. The surrounding halo appears less concentrated with a gradual fading of light from the center outwards. The overall morphology seems elliptical in nature, with a slight elongation visible. There is no distinct spiral arm structure or obvious signs of recent major merger events. The color gradient may indicate a degree of metallicity variation across the galaxy. There are no clear signs of active star formation within the galaxy's disk, further supporting the idea of a more evolved system. A faint outer halo may be present though the resolution limits more detailed analysis.
