The galaxy presents as a somewhat smooth, centralized object. Its overall form appears moderately elliptical in shape. There is a subtle color gradient visible, transitioning from a slightly bluer hue in the central region to a redder tone toward the outer edges. While generally smooth, subtle internal features such as a faint disk-like structure or minor disturbances cannot be entirely ruled out based on this image alone. Signs point toward an older stellar population as the dominant contributor to the overall luminosity. There is no clear indication of ongoing major star formation, nor is there any indication of a major merger occurring. 
