The galaxy presents as a single, relatively smooth concentration of light. It appears roughly elliptical in shape, displaying a high degree of circularity. The primary color is a pronounced yellow-orange hue, which is consistent with a stellar population dominated by older, redder stars. There are hints of faint, diffuse structures around the main body, but no clear spiral arm features or significant dust lanes are apparent. Close examination reveals minimal evidence of ongoing star formation within the galaxy itself. There is no obvious central bulge structure, giving it an overall diffuse appearance. The galaxy does not appear to be undergoing any major mergers or tidal disturbances.
