The galaxy presents as a well-defined elliptical shape with a bright, concentrated core. There is a noticeable color gradient, shifting from a yellowish-white center to a faint greenish hue in the outer regions. The galaxy exhibits a high degree of smoothness, with no distinct spiral arm structures or dust lanes visible. The light distribution appears to be centrally concentrated, with a rapid decline in brightness from the core outwards. It looks like a relatively undisturbed system, showing no significant signs of tidal interactions or recent merger events. Based on the color profile, there is a high probability of older stellar populations with less ongoing star formation.
