The galaxy appears as a single, unresolved, centrally concentrated object. It exhibits a smooth, elliptical morphology, with a high degree of roundness. No distinct features such as spiral arms or a prominent disk component are discernible. There is no evidence of significant ongoing merger activity or major disturbances in its structure. The galaxy presents a concentrated color profile, showing relatively low star formation. Overall, it appears to be a relatively quiescent system, likely a mature elliptical galaxy dominated by an older stellar population.
