The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. The light distribution is concentrated towards the center, with a gradual decrease in brightness outwards. The core exhibits a bright, relatively concentrated glow. The overall color appears slightly redder than the surrounding field objects. There is a slight asymmetry or a possible minor distortion in the galaxy's structure, with some suggestion of faint tidal features or a subtle disturbance in its outer regions. There are no clearly defined spiral arms or a prominent central bar. Some potential evidence for merging activity could be present, though more data would be required to confirm this.
