The galaxy presents a largely smooth and rounded morphology, appearing elliptical or lenticular in nature. There is a central concentration of light, suggesting a nucleus or bulge component. The radial light profile decreases gradually from the core, exhibiting a diffuse halo extending outwards. There is a subtle color gradient visible, shifting from slightly yellower hues in the central region to marginally bluer tones towards the outer edges of the galaxy. No distinct spiral arms, bars, or significant dust lanes are discernible. The galaxy appears relatively undisturbed, showing no clear evidence of recent major merger events or tidal features.
