The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. Its overall shape is somewhat elongated, approaching a cigar-like appearance. There is no prominent spiral arm structure visible; instead the light is rather diffuse. The galaxy exhibits a color gradient, with a slightly bluer hue at the center fading to redder tones towards the outer edges. This color variation could signify older stellar populations dominating the outer regions and possible ongoing, although weak, star formation within the core. There is no indication of tidal disturbances or interaction with another galaxy. The lack of clear morphological features and the smooth, diffuse light indicate a relaxed system that has likely undergone significant dynamical evolution.
