The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology is largely spheroidal, exhibiting a high degree of roundness. There is little to no evidence of spiral arms or a distinct disk structure. The light distribution appears fairly uniform across the galaxy, lacking strong features such as prominent star-forming regions or dust lanes. No major disturbances or signs of ongoing or recent merger activity are observed. The color profile indicates that the galaxy is primarily composed of older stellar populations, with minimal recent star formation, evidenced by its redder hue.
