The galaxy presents as a centrally concentrated elliptical morphology, with a smooth, diffuse light distribution. There is a noticeable color gradient, transitioning from a yellowish-white core to a bluer periphery, suggesting the presence of younger stellar populations in the outer regions relative to the core. The isophotes appear largely regular, with only minor deviations from perfect ellipticity, indicating a relatively relaxed dynamical state. There is no evidence of prominent spiral arms, bars, or tidal features, suggesting no recent major merger events, although there may be minor disturbances. The observed light profile suggests a mature galaxy with a significant bulge component, and possibly a weak star formation rate in the outer regions. Overall, this appears to be a galaxy that is mostly spheroidal in shape, with an intermediate roundness.
