The galaxy appears to be an elliptical galaxy with a generally smooth morphology. Its shape is somewhat elongated, with a notable lack of defined spiral arm structures. The light is concentrated in the center, suggesting a dense galactic nucleus. There is a gradual decrease in luminosity moving outwards from the center. The galaxy exhibits a redder hue, implying an older stellar population with a relative absence of recent star formation. There's a slight suggestion of very minor disturbance at the edges of the disk, though it appears very subtle.
