The galaxy presents as a relatively smooth, elongated elliptical structure. Its central region exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, bluish extensions emanate from this central region along the major axis, which may suggest the presence of younger stars or areas of active star formation, though the smoothness of the galaxy suggests that it is not forming many stars. The galaxy displays no obvious spiral arms or strong dust lanes, further suggesting a relatively featureless morphology. There appears to be a slight warp or bending visible in the galaxy's extended disk, hinting at a possible past interaction or tidal disturbance. The shape is significantly elongated, but no prominent central bulge is visible. 
