The galaxy presents as an elliptical morphology, with a high degree of smoothness observed across its light profile. The central region exhibits a concentration of light, appearing somewhat rounded. There is a slight elongation suggesting it is not perfectly spherical. While no major disturbances are apparent, there might be minor irregularities in the outer regions. The galaxy appears to be a relatively quiescent system with a subdued rate of star formation. The color gradient suggests a population of older stars, with a notable absence of strong blue light indicative of recent or ongoing star formation.
