The galaxy presents a predominantly smooth morphology with an elliptical shape. The central region exhibits a high concentration of light, indicating a bright, dense core. The light gradually diffuses outwards from the core, forming a surrounding halo. This halo is characterized by a relatively even distribution of light with only small amounts of detail in the textures. The galaxy is mostly smooth, with no apparent spiral arm structures or significant dust lanes observed. The colour of the galaxy appears to be on the redder side, which could point to an older stellar population, indicating lower levels of ongoing star formation. The galaxy seems to be isolated, displaying no obvious signs of recent or ongoing interaction with other galaxies.
