The galaxy appears to be an elliptical type, exhibiting a generally smooth and featureless morphology. It is elongated in shape, with a cigar-like aspect ratio. The color gradient suggests a concentration of older, redder stars toward the center of the galaxy, which transitions to a bluer hue in the outer regions. There is no apparent spiral structure or significant dust lanes visible in this image. The light distribution seems relatively even, without signs of major mergers or tidal disturbances, though some minor asymmetry cannot be ruled out given the resolution.