The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, concentrated luminosity profile. The overall shape is elongated, showing a cigar-like form, rather than being circular. The central bulge is prominent and exhibits a yellowish hue, suggesting a population of older stars. The outer regions display a subtle color gradient transitioning to redder tones, which could be an indication of aging stellar populations or dust obscuration. There may be some features or disk that is obscured by the intense light and angle it is tilted. There is no evidence of major disturbances or merging activity in this image.
