The galaxy appears to be largely elliptical in nature. It exhibits a relatively smooth light distribution, with a concentration of light towards the center. The overall color profile indicates a greater presence of older stellar populations, with a redder hue. There is evidence of some structural disturbance or interaction, possibly tidal features or minor asymmetries in the outer regions. The galaxy is more spherical than it is disk-shaped, although there is evidence of some disk features present. Additionally, the galaxy shows evidence of a potential ongoing or past merger event; structural distortions or extended tidal tails are visible, indicating gravitational interactions with another galaxy.