The galaxy presents as a luminous object with a somewhat elliptical morphology. It exhibits a high degree of central concentration, with a bright, yellowish core that suggests an older stellar population. Moving outward from the core, the color transitions towards a more bluish hue, indicating the presence of younger, hotter stars in the outer regions. The overall structure appears relatively smooth, but there is a slight asymmetry suggesting the presence of a disk or minor disturbance. No prominent spiral arms are visible, but subtle features hint at possible underlying structure. Based on its colour and structure, the galaxy can be classified as an early-type spiral galaxy, possibly influenced by interaction with a smaller companion in the background.