The galaxy presents a generally smooth and rounded morphology, suggesting an elliptical or lenticular classification. The light is concentrated towards the center, forming a bright nucleus that decreases in intensity outward. There are no readily apparent spiral arms or distinct disk-like features. The color profile seems to indicate a presence of older stellar populations. The overall appearance implies a relatively evolved system, with a lack of significant recent star formation activity. There are no strong indications of any major ongoing merger events or tidal disturbances.
