The galaxy presents as an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, indicative of an older stellar population. The galaxy appears yellowish-white in color, suggesting a lack of significant ongoing star formation and a dominance of older, redder stars. There is a subtle elongation to its shape, transitioning between a rounded and cigar-shaped structure. No prominent spiral arms or dust lanes are discernible. There does not appear to be any signs of any interactions or mergers occurring.
