The galaxy presents as a roughly elliptical, diffuse object with a high degree of central concentration. The core exhibits a bright, almost stellar-like, appearance transitioning into a smoother, extended halo. The outer regions appear less defined, fading into the background sky. The color gradient shows a shift towards redder hues in the central regions, indicating potentially older stellar populations and/or higher dust content there. There is some indication of tidal disturbances present. The galaxy may be a candidate for further investigation into galactic mergers.
