The galaxy presents a predominantly smooth, elliptical morphology with a high degree of roundness. The central region exhibits a concentrated, bright core indicative of a significant stellar population and/or active galactic nucleus. The color profile appears redder in the central bulge region, suggesting a dominant population of older stars and relatively low ongoing star formation. There is a very slight suggestion of a minor disturbance in its shape and structure. Overall, this galaxy appears to be a relatively evolved system.
