The galaxy presents a predominantly smooth morphology. It appears largely elliptical in shape, exhibiting a high degree of central concentration. The light distribution decreases radially from a bright, saturated core. There is some indication of a faint, diffuse halo surrounding the central region, however, its boundaries are ill-defined. No distinct features such as spiral arms, bars, or tidal tails are discernible. There is no noticeable dust lane or any other signs of significant dust obscuration. The overall color appears relatively red, suggesting an older stellar population with a low current star formation rate. There is no apparent indication of any ongoing merger activity or significant galactic interaction.
