The galaxy presents as a relatively smooth, elliptical structure. Its overall shape appears somewhat flattened, though not dramatically elongated. The color is generally yellowish, suggesting a population of older stars. There is a slightly brighter, more compact core region, indicating a concentration of stellar mass towards the galactic center. There does not appear to be any distinct spiral arm structure or significant dust lanes visible in this image. A slight asymmetry might indicate minor gravitational interactions or recent accretion events. There is little evidence of ongoing, active star formation in the galaxy.
