The galaxy presents as a somewhat elliptical, smooth structure, displaying a dominant yellow-orange hue at its core, suggesting an older stellar population. There appears to be a distinct, irregular feature, possibly a tidal tail or disturbed dwarf galaxy, exhibiting a bluish tint, indicative of recent star formation or a population of younger, hotter stars. The main body of the galaxy shows no clear spiral arm structure and a high degree of central concentration, further supporting its classification as an early-type galaxy. Evidence of ongoing merger activity is not readily apparent in the main galactic structure, but is implied by the presence of the blue structure nearby.
