The galaxy presents as a relatively smooth, elliptical morphology. Its overall color profile indicates an older stellar population. A bright, concentrated central bulge dominates the structure, with the luminosity appearing to gradually decrease towards the outer regions. There is a slight elongation in its shape, deviating from perfect circularity. No distinct spiral arm structures or prominent dust lanes are discernible. Subtle color variations can be observed, transitioning from a yellow-orange hue in the core to a slightly bluer tint in the outskirts, suggesting potential variations in stellar age or metallicity across the galactic disk. There does not appear to be a close merger, and the overall galaxy appears to be largely undisturbed.
