The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated morphology with a bright core, suggesting a high stellar density in the nuclear region. The overall shape is generally round, lacking any obvious spiral arm structures or significant disk component. There are no apparent signs of major tidal disturbances or ongoing mergers, although a very slight asymmetry or minor irregularity cannot be entirely ruled out. Color gradients suggest the presence of an older stellar population within the galaxy, with a possible moderate level of star formation.
