The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. The central region exhibits a concentration of light, appearing nearly spheroidal in shape. The color gradient transitions from a yellowish hue at the core to a bluer periphery, hinting at potential variations in stellar populations or dust distribution within the galaxy. There is no apparent spiral structure or bar visible in the image. Slight irregularities in the outer regions could indicate minor tidal interactions or recent accretion events, though the overall structure suggests a relatively relaxed system.
