The observed galaxy appears as a diffuse, centrally concentrated object with a generally smooth morphology. It exhibits a moderate ellipticity, with the overall shape deviating slightly from a perfect circle. The galaxy displays a color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population, while the outer regions have a slightly bluer hue indicating a younger stellar population. There appears to be a second, smaller galaxy in close proximity to the larger one.

There are indications of possible tidal disturbances or minor interactions occurring in this galaxy system. This could be from a recent or ongoing merger. There also appears to be some diffuse light extending away from the main body of the galaxy, potentially indicating tidal tails or stripped material. The galaxy's overall appearance is consistent with a relatively massive system that is either undergoing interactions or has recently experienced a merging event. The estimated redshift indicates it is a relatively distant object.
