The galaxy appears as a moderately bright, elliptical or lenticular system exhibiting a generally smooth morphology. The light profile is centrally concentrated with a gradual falloff in surface brightness towards the outer regions, suggesting an older stellar population. There is a slight asymmetry, which may indicate a minor interaction or internal disturbance. The core is distinctly yellow or orange, potentially indicating a population of older, redder stars and relatively low levels of recent star formation. Faint red features are present in the extended halo of the galaxy. The overall structure suggests a system that has largely completed its major mergers and is now in a relatively quiescent phase of evolution.
