The galaxy presents an elongated, elliptical morphology. The central region exhibits a high degree of luminosity, suggesting a dense stellar population or active galactic nucleus. The light distribution becomes more diffuse towards the outer regions of the galaxy. There is a subtle colour gradient, transitioning from a yellowish-white core to a redder hue in the extended halo. This may indicate older stellar populations dominating the outer regions. No prominent spiral arm structures are visible, implying a relatively smooth and featureless structure. There is no apparent evidence of ongoing major mergers or significant tidal disturbances in this image. 
