The galaxy presents a generally smooth morphology with a dominant central bulge. The bulge appears approximately spheroidal and exhibits a yellowish-orange hue, suggesting a population of older, cooler stars. Surrounding the bulge is a fainter, bluish disk component. This disk is not sharply defined and lacks prominent spiral arm structure. There is a slight elongation to the galaxy, indicating it is not perfectly spherical. The overall color profile suggests that the galaxy is undergoing a modest amount of star formation, with the blue regions potentially indicating younger stellar populations within the disk. There is no visually apparent active galactic nuclei or dust lanes, and the galaxy appears relatively undisturbed. The image doesn't suggest a major ongoing merger or significant tidal distortions.
