The galaxy presents as a relatively compact object. Its morphology appears largely smooth, with a somewhat elliptical shape, trending towards round. The light distribution suggests a high degree of central concentration. There is a hint of some asymmetry present, possibly indicating a minor gravitational disturbance, such as a faint tidal tail or subtle distortion in the outer regions. The galaxy exhibits a yellowish-red color, suggesting an older stellar population, and a relatively low rate of ongoing star formation. It does not appear to be actively merging with another galaxy, although a past interaction cannot be entirely ruled out based on the subtle morphological features. The overall impression is of a massive, evolved system with a considerable stellar mass.
