The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a high degree of luminosity, with a gradual decrease in brightness moving outward towards the edges. There's a slight yellow-orange hue, suggesting an older stellar population dominating the light output. No distinct spiral arms or significant dust lanes are discernible. Overall, the galaxy appears well-defined and isolated, without apparent signs of recent major merger events or tidal disturbances. The lack of blue light implies a low rate of current star formation. The object has a generally rounded shape, but there may be a very slight cigar shape to the overall morphology.
