The galaxy presents as a relatively bright, single object with a smooth, centrally concentrated morphology. It appears somewhat spheroidal in shape, exhibiting a high degree of roundness. There is no apparent evidence of spiral arms, bars, or other distinct disk-like structures. The galaxy exhibits a color gradient, appearing more yellow or golden in the central regions, suggesting an older stellar population. There is no obvious indication of recent or ongoing major merger activity, tidal tails, or other significant disturbances in its structure.
