The galaxy appears as a relatively smooth, elliptical-like structure with a distinct central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter, diffuse blue emissions are visible in the surrounding areas, possibly indicating regions of ongoing, albeit subdued, star formation. The galaxy's overall morphology suggests it is not a late-type spiral. The galaxy has a somewhat intermediate axis ratio but overall appears mostly rounded. There are no obvious signs of tidal tails or major disturbances, implying it is likely not undergoing a major merger event currently. The galaxy demonstrates a red shift, indicating that it is not nearby. The size is roughly 5 kpc across.
