The galaxy presents a primarily smooth morphology, with a generally elliptical shape. It appears largely undisturbed, showing no strong signs of ongoing major merger activity. The color distribution suggests an older stellar population, with a higher concentration of light in the redder wavelengths. Based on color, there is little active or current star formation in the region. The galaxy shows a high level of concentration, and is generally well-defined in shape. There is a fainter structure attached to the galaxy, and it is difficult to determine if it is a part of the galaxy or a background object.
