The galaxy presents as a relatively compact, elliptical-like structure with a smooth, diffuse light distribution. It appears to be generally round in shape. The galaxy's color is predominantly yellow-orange, suggesting an older stellar population with a reduced rate of star formation. There is no clear evidence of spiral arms, bars, or significant dust lanes. While appearing largely undisturbed, subtle irregularities in the outer regions may indicate minor tidal interactions or past mergers. Based on the limited available image data, this is likely a massive galaxy with a significant stellar mass.
