The galaxy presents a primarily smooth morphology, exhibiting a significant central bulge region that dominates its overall appearance. The color profile of the galaxy is characterized by a yellowish-orange hue, suggesting a population of older stars. The shape is somewhat elliptical, verging towards a disc, with a slight elongation observed. There are no obvious signs of strong spiral arm structures, though a faint disk structure may be present. The galaxy appears relatively undisturbed, with no prominent tidal tails or other indicators of recent major merger events. There is some hint of slightly bluer features or small disk near the edges, suggesting low-level star formation. Overall, the galaxy appears to be a relatively massive and passively evolving system.
