The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity toward the outer regions. There appears to be a slight elongation, suggesting it is not perfectly spherical, but rather somewhat flattened. The color profile indicates a possible older stellar population, with a dominant yellowish-white hue at the core transitioning to slightly bluer tones in the outskirts. No distinct spiral arms or prominent dust lanes are discernible within this resolution. There are no apparent signs of major disturbances or interactions with other galaxies.
