The galaxy presents a largely smooth and centralized light profile, suggesting a relatively evolved system. It appears moderately elliptical, deviating slightly from a perfect circular shape. The galaxy displays a color gradient, appearing more yellow-white towards its core and trending towards redder hues in its outer regions. There is some evidence of a possible minor disturbance or merging event. A fainter, redder structure appears closely associated with the primary galaxy, potentially indicating a smaller galaxy in the process of merging or experiencing a close tidal interaction. Overall, the object seems to be a luminous galaxy at a considerable distance, possibly a massive elliptical galaxy with ongoing or recent merger activity. The galaxy's color suggests a moderate amount of ongoing star formation or the presence of an older stellar population.
