The galaxy presents a generally smooth morphology, with a dominant central bulge. The light distribution appears relatively concentrated, fading gradually outwards. The galaxy's color is predominantly yellowish-orange, suggesting a stellar population that is older and redder than actively star-forming galaxies. There are hints of underlying disk features, however these are subtle. No prominent spiral arms or distinct dust lanes are visible in the image. The galaxy does not appear to be undergoing any major merging activity.
