The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be nearly spherical. It exhibits a concentrated, bright central region, likely indicating a bulge component. The galaxy's color is predominantly a yellow-orange hue, suggesting an older stellar population. There appears to be little evidence of ongoing star formation or spiral arm structures. The outer regions gradually fade into the background sky, indicating a lack of sharp boundaries. There is no evidence of major disturbances or merging activity.
