This galaxy exhibits a relatively smooth, elliptical morphology. It is characterized by a concentrated central bulge, which appears yellowish in color, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, with a bluer hue indicative of younger, hotter stars and ongoing star formation, albeit at a low rate. There are slight disturbances evident within the disk, although these features are subtle. Overall, the galaxy presents a low likelihood of recent major merger activity, but some minor disturbances may be present.
