The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits an overall elliptical shape, and its color is slightly redder in the central region, suggesting an older stellar population. The outer regions of the galaxy appear fainter and slightly bluer, hinting at the presence of younger stars or a lower concentration of stars. There is no obvious dust lane or spiral arm structure visible in this image. Slight asymmetries exist, but they are not indicative of any major ongoing merger or significant interaction. Overall, the galaxy appears to be a relatively isolated and evolved system.
