The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. Its color appears redder in the image, suggesting an older stellar population and a possible suppression of recent star formation. The shape is generally round with some irregularity. There may be minor disturbances or interactions occurring, as evidenced by some asymmetric features. The galaxy exhibits characteristics suggestive of a substantial mass. Based on the observed features, the galaxy likely experienced a major merging event in the past, as evidenced by its irregular appearance.
