The galaxy presents as a single, centrally concentrated object with a smooth light profile. It is largely featureless, exhibiting a high degree of symmetry. There is little evidence of spiral arms or dust lanes. The galaxy appears nearly circular in shape. There is a very slight indication of deviation from perfect roundness, but it is subtle. The color gradient appears consistent with an older stellar population. There are no signs of any major ongoing merger activity, though a minor tidal interaction cannot be ruled out based on this image alone. The galaxy's luminosity is relatively high, which could indicate a substantial stellar mass.
