The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellowish hue, suggesting a population of older stars. There is a slight elongation to the galaxy's shape, but it is generally round. No distinct spiral arms or prominent dust lanes are visible. Faint blue hints can be seen in the outer regions, which may indicate recent star formation, though at a low rate. The galaxy shows no obvious signs of major mergers or tidal disturbances, though minor irregularities cannot be ruled out at this resolution.
