The galaxy presents as a generally elliptical morphology, characterized by a smooth light distribution with no discernable spiral arm structure or bar. The central bulge region appears concentrated and displays a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, fading into a less distinct halo. Subtle color gradients can be observed, with a slight shift towards bluer tones in the fainter, more diffuse regions surrounding the core. There is no visual evidence of ongoing major merger activity or significant tidal disturbances affecting the overall structure. The galaxy appears relatively isolated and undisturbed.
