The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated with an elliptical shape, with no obvious spiral arm structure visible in this image. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in its inner regions to redder tones in its outer parts. This suggests the presence of older stellar populations dominating the outer areas. The absence of distinct features like dust lanes or prominent star-forming regions indicates a likely lack of significant ongoing star formation activity. There are no visual signs of any tidal disturbances or interactions with neighboring galaxies, pointing toward a relatively undisturbed evolutionary history.
