The galaxy appears as a generally smooth, elliptical-like structure. There is a dominant central bulge that exhibits a yellow-orange hue, suggesting an older stellar population likely dominated by red giant stars. Faint hints of a disk-like component are present, though these features are not well-defined. The overall shape is somewhere between round and elongated. Some irregular features are observed, hinting at a possible interaction or merger event. There appears to be a slight disturbance in the galaxy's morphology. Star formation appears to be relatively low, which supports the prevalence of an older stellar population. The galaxy does not show any prominent spiral arm structures or dust lanes.
