The galaxy appears to be an elliptical type, exhibiting a generally smooth, concentrated morphology. There are no obvious spiral arms or distinct disk features visible. It displays a somewhat elongated shape, deviating slightly from a perfectly circular form. The galaxy's color profile suggests an older stellar population, with a redder hue. There are signs that this galaxy could be experiencing minor interactions, with the presence of potential disturbances. The overall appearance suggests a system undergoing or having undergone a merger event, although the degree of disruption seems relatively subdued.
