The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly spherical. There's a definite concentration of light toward the center, suggesting a prominent galactic bulge. The galaxy exhibits a color gradient, with the central region appearing more yellowish-orange, indicative of an older stellar population. The outer regions of the galaxy show a bluer hue, which is likely due to the presence of younger, hotter stars, but is less pronounced. There's no obvious spiral arm structure or dust lanes visible at this resolution. The overall morphology suggests a galaxy that has largely completed its star formation, but with perhaps some ongoing activity in its outer regions, although the rate is expected to be low. There is no significant morphological evidence of a recent major merger event or significant tidal disturbance. The shape is somewhere in-between a sphere and a cigar.
