The galaxy presents as a generally smooth, centrally concentrated object. Its color appears yellowish, suggesting a population of older stars and a relative lack of ongoing, intense star formation. The galaxy exhibits a somewhat elliptical morphology, appearing mostly round but possibly slightly elongated along one axis. There is no strong evidence of spiral arms or a prominent disk structure. Faint irregularities or subtle disturbances in the outer regions might be present, which could indicate minor gravitational interactions. The galaxy appears to be a relatively massive system with modest star formation rates.
