The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central region with a diffuse halo extending outwards. The light distribution is elongated, suggesting a cigar shape rather than a perfect sphere. Color gradients are present, with the core appearing a more intense yellowish-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy show a bluer tint. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. No obvious signs of tidal disturbances or active galactic nuclei are observed. The galaxy is not obviously undergoing a major merger event, although there is slight asymmetry.
