The galaxy presents as a relatively smooth, centralized object with a diffuse halo. The core appears to be of higher luminosity, with a noticeable yellow-orange hue, suggestive of an older stellar population. There's a general lack of discernible spiral arms or defined structures, indicating it's likely an elliptical or lenticular galaxy, appearing more rounded than elongated. The absence of major disturbances points to a non-merging, relatively quiescent state. The halo exhibits a smooth, gradual decline in intensity from the core, without any prominent tidal features. The overall color suggests evolved stellar populations and potentially lower levels of ongoing star formation.
