This galaxy presents a generally smooth, elliptical morphology. The galaxy core exhibits a bright, concentrated luminosity, indicative of a dense stellar population. The overall color appears reddish-gold, suggesting an older stellar population with a low rate of ongoing star formation, further supporting the classification as an elliptical galaxy. There may be some evidence of minor disturbances in the outer regions, possibly indicating past or ongoing interactions, although a significant portion of the light is still emanating from a relatively undisturbed bulge. The galaxy appears somewhat rounded in shape. There is the suggestion that the galaxy is potentially undergoing a merger, perhaps with a smaller object, but this may also be an artifact.
