The galaxy presents a predominantly smooth morphology with a high degree of central concentration. It appears elliptical in shape, tending towards round, with a very slight elongation along one axis. The light distribution is generally even, with a bright, yellowish core. This core suggests an older stellar population dominating the central regions. Fainter, diffuse bluish light is visible in the outskirts indicating a possible younger stellar population or some low-level star formation occurring in the outer regions. There is a hint of minor disturbances within the galaxy’s morphology, but its structural components are generally coherent, with no clear indications of a major ongoing merger. Overall, the galaxy exhibits characteristics consistent with a relatively quiescent state.
