This galaxy presents an overall elliptical morphology, exhibiting a high degree of central concentration and a smooth luminosity profile. The core region appears bright, gradually fading towards the outer edges of the galaxy. The isophotes appear generally elliptical but there are hints of some minor disturbances in the outer regions, perhaps suggesting a past interaction or merger event. A faint, extended halo surrounds the central body. The galaxy's color index is consistent with a population of older stars with only a few regions of modest recent star formation. There may also be some signs of a merger with a smaller dwarf galaxy, possibly indicating an ongoing hierarchical growth process.
