The galaxy presents as a relatively smooth, elliptical morphology. Its light is concentrated in a central bulge, appearing with a yellowish-orange hue, suggesting an older stellar population. The outer regions exhibit a gradual decrease in luminosity, fading into the background sky. There's a slight elongation, but overall, the galaxy appears largely spheroidal. No distinct spiral arm structures or prominent dust lanes are discernible in this image. Based on the color and morphology, this galaxy is likely a mature system with a low star-formation rate. There is no obvious sign of any major merging event.
