The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears largely elliptical, exhibiting a near-circular profile with minimal discernible features such as spiral arms or a prominent disk. The luminosity is highest at the core, gradually diminishing towards the outer regions. There is no clear evidence of tidal distortions, ongoing mergers, or significant disturbances in its structure. Based on its color and morphology, this galaxy likely contains an older stellar population and is not undergoing active star formation.
