The galaxy presents as an elliptical morphology, elongated in shape. There appears to be a concentration of older stellar populations, indicated by the reddish-yellow hue emanating from the galaxy's center and extending outwards. The outer regions display a fainter, more diffuse light, suggesting a gradual decline in stellar density from the core. There are also signs of tidal disruption, which points to a possible merger with another galaxy in the past. Overall, the galaxy seems to be relatively quiescent in terms of star formation.
