The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. The core region exhibits a reddish-orange hue, potentially indicative of an older stellar population and/or dust obscuration. Moving outward from the core, the color shifts to a greenish-yellow, suggesting a slightly younger stellar population than that of the core, though not substantially so. The overall structure appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The galaxy appears to be a relatively massive system, based on its brightness. The shape is elongated, with a cigar-like appearance, suggesting that it is not a face-on system. The outer regions of the galaxy fade gradually, with no sharp cut-off in the stellar density. There are no prominent spiral arms or bar structures visible in the image. Star formation is likely occurring at a very low rate, if at all.
