The galaxy presents a flattened, elliptical morphology, viewed at an oblique angle. It exhibits a smooth, centrally concentrated luminosity profile with a bright, yellowish core, possibly indicative of an older stellar population. The surrounding disk appears less luminous and displays a slightly bluer hue, suggesting the presence of a younger stellar population and ongoing star formation activity. No prominent spiral arms or distinct dust lanes are discernible. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy's estimated physical size suggests it is a moderately large system.
