The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge exhibiting a yellowish hue. The overall structure displays a high degree of circularity. There is no readily apparent spiral arm structure or significant dust lane obscuration. Subtle color variations are visible within the galaxy's profile, with a slightly bluer, more diffuse halo surrounding the brighter, yellower core. There are no obvious signs of active galactic nuclei or any ongoing major merger events, although a possible minor disturbance cannot be entirely ruled out. Based on its color profile, the galaxy likely contains a population of older stars with relatively low current star formation. The galaxy exhibits an estimated size of approximately 6 kiloparsecs.
