The galaxy presents as a somewhat elliptical structure, with a central bulge that appears more luminous and exhibits a yellow-orange hue, suggesting an older stellar population. The surrounding disk shows a bluer tint, potentially indicative of ongoing star formation. The galaxy lacks any distinct spiral arm structure and appears relatively smooth in texture. There's no visible evidence of a significant ongoing merger or tidal disturbance, but it could have undergone minor disturbances. The galaxy's light is somewhat dispersed, indicating it is likely a moderate to high mass galaxy.
