The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The morphology is predominantly spheroidal, exhibiting a notable lack of spiral arms or a distinct disk component. The galaxy's color profile displays a dominant yellowish hue, potentially indicative of an older stellar population with a lower rate of current star formation activity. There is a subtle bluer tint at the periphery of the galaxy, which may be due to the presence of a younger stellar population in the outer regions or be a product of image processing artifacts. No major tidal disturbances or interactions with neighboring galaxies are visually apparent.
