The galaxy appears to be an elliptical galaxy, exhibiting a smooth, elongated shape with a high degree of central concentration. Its morphology is cigar shaped. There is a discernible color gradient within the galaxy, shifting from a yellowish hue in the center to a bluer color in the outer regions. This could indicate a difference in stellar populations, with older, redder stars concentrated in the center, and younger, bluer stars more prevalent in the outer parts. There is minimal evidence of any significant disturbances or merging events affecting the galaxy's overall structure.
