The galaxy presents a generally smooth morphology, with an elliptical-like structure dominating the visual appearance. There appears to be a slight elongation in the structure, though it is mostly round. A yellowish hue permeates the central region of the galaxy, suggesting an older stellar population. A small degree of bluer color in the surrounding periphery indicates a small amount of ongoing star formation. Faint reddish hues on one side suggest slight dust absorption or potentially a population of older stars. Based on its morphology, this galaxy is likely a fairly massive system, but with only a minor amount of current star formation. The overall structure appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions, but there is the potential for some minor disturbances given the color fluctuations.
