The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge that is bright and concentrated, appearing yellowish in color, suggesting an older stellar population dominating this region. Moving outward from the core, the light gradually diffuses into a fainter halo. Subtle color variations are observed in the outer regions, with hints of bluer hues, possibly indicating some ongoing, albeit limited, star formation. There's a slight elongation to the galaxy's shape, but it is overall relatively round. No distinct spiral arms or prominent dust lanes are apparent. There might be slight irregularities, which could indicate minor gravitational interactions, but these are not particularly pronounced.
