The galaxy appears as a relatively smooth, elliptical-shaped structure. It exhibits a concentrated central bulge, with a noticeable decrease in luminosity moving outwards from the center. The color appears somewhat uniform across the galaxy, suggesting an older stellar population. There is no obvious spiral structure or dust lane. The edges are indistinct and fade smoothly into the background sky, indicating a gradual decrease in stellar density. The overall morphology suggests a relaxed system without signs of significant recent merger activity or active star formation. The galaxy is nearly circular, indicating it is closer to an E0-E1 elliptical.
