The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light is dominated by yellow and red hues, suggesting an older stellar population with minimal ongoing star formation. It exhibits a high degree of roundness with no obvious spiral arms or disk-like features. There is no visual evidence of any major mergers or tidal disturbances, although a very slight asymmetry is possible. The galaxy appears relatively isolated, with no immediately apparent companion galaxies or interacting structures. Based on color, the galaxy appears to be quite massive.
