The galaxy presents as a relatively smooth, elliptical morphology, exhibiting a high degree of central concentration. Its color profile appears generally blue-white, indicating the presence of a younger stellar population compared to a purely red and dead elliptical. The overall structure shows minimal evidence of spiral arms or other distinct features, instead resembling a spheroidal shape. There are no obvious signs of significant tidal interactions or ongoing merger events, although a subtle asymmetry on one side might suggest past gravitational disturbances. The galaxy displays a noticeable radial brightness gradient, with a brighter, more intensely luminous core gradually fading into the outer regions. Given the lack of prominent dust lanes or extended gas clouds, the rate of ongoing star formation is likely low. The smooth texture and rounded appearance suggests a dynamically relaxed system.
