The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated with a noticeable radial gradient, transitioning from a brighter, yellower core to a slightly dimmer, redder halo. There is a subtle extension to the redder halo, but no distinct spiral arm structure or bar feature is visible. The galaxy appears relatively undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. The color suggests an older stellar population, with relatively little ongoing star formation. The object appears to be generally round. Any disturbances seem very minor if present at all.
