The galaxy presents as an elongated, cigar-shaped object, consistent with an elliptical morphology. There is a central, brighter region suggestive of a higher stellar density bulge, surrounded by a more diffuse halo. The color appears relatively uniform across the galaxy with a hint of redder hues, potentially indicating an older stellar population and a lower rate of on-going star formation. No distinct spiral arm structures or dust lanes are discernible in the image. The overall smoothness of the light distribution further supports its classification as an elliptical galaxy. There is no obvious evidence of recent or ongoing major mergers, though the slight asymmetry of the outer halo may suggest past minor interactions.
