The galaxy presents as a fairly smooth, elliptical morphology. It exhibits a concentration of light towards the center, suggesting a well-defined nucleus or core. While the overall structure appears generally smooth, subtle color variations can be observed across the galaxy's body. The central region has an enhanced yellow/red hue in comparison to bluer outer regions, which potentially indicates older stellar populations concentrated in the center and regions of more recent star formation in the outskirts. The shape is generally rounded, but there are some hints of elongation. There is no evidence for ongoing major merger activity or strong tidal disturbances, though subtle irregularities may indicate minor interactions. Overall the galaxy appears to be in a relatively quiescent state.
