The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution. It presents a cigar shape, indicating a significant ellipticity. The light is more concentrated towards the center, with a gentle fading towards the edges. There's a subtle hint of a disk-like structure, but the dominant morphology is smooth. The color gradient suggests older stellar populations, primarily composed of yellow and reddish hues, with a faint bluer region on the edges. This indicates a relatively low star formation rate. There is a slight asymmetry in the light distribution. The galaxy does not show signs of strong spiral arms or active galactic nuclei activity. It is likely to be a relatively massive galaxy, exhibiting a small amount of star formation.
