The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its light profile increases towards the center, peaking in a bright, compact core region. The galaxy shows an overall elongated shape, not perfectly spherical. The outer regions fade gradually, suggesting a diffuse halo structure. There is a slight hint of bluer light in the outer regions compared to the yellow-white hue of the core, possibly indicating some degree of ongoing star formation. There are no apparent spiral arm structures or major disturbances visible within the galaxy's morphology. The galaxy does not appear to be undergoing a major merger, however there is a slight disturbance with a hint of possible merging with a smaller companion galaxy, as the outer regions are not completely smooth.
