This galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a slightly elongated morphology. The primary color appears to be a yellowish-orange hue, suggesting an older stellar population with relatively low levels of ongoing star formation. There appear to be signs of a possible ongoing or recent merger event, with two distinct, bright central concentrations that hint at multiple galactic nuclei. Given the high fraction of light coming from older stars and the potential merger activity, the galaxy likely has a high stellar mass.